Details on Acronym: H
H (Higgs) (Not yet in Simbad) ***** Avoid the usage of H, prefer Hig
Details on Acronym: H
H (Hubble) ***** Avoid the usage of H, prefer BASW Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (Harten) ***** Avoid the usage of H, prefer [BHJ77] Originof the Acronym: L (1980A&A....90..246I)
Details on Acronym: H
H (HDF) ***** Avoid the usage of H, prefer [CSS2000] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H (HI Hole) ***** Avoid the usage of H, prefer [DD90] Originof the Acronym: L (2001PASJ...53..663O)
Details on Acronym: H
H (Hyland+) ***** Avoid the usage of H, prefer Dor Originof the Acronym: L (1998A&A...331..857J)
Details on Acronym: H
H (HEAO satellite)= (HEAO) Write:<<H HHMM+DD>>
<<H HHMM+DDd>> N: 60+114 Object:(X) (SIMBAD class: X = X-ray Source) Note:1979ApJS...40..657M: N=60, 47 are new sources, All sky, Energy 3-17 keV. 1983ApJS...51....1N: N=114, 54 were previously undiscovered and 32 remain unidentified. The catalogue contains a listing of all counterpart identif. and a cross-reference to all HEAO 1 A-2 low energy detector team publications on the catalogue sources complete through the end of 1981. Ref:=1979ApJS...40..657M byMARSHALL F.E. , BOLDT E.A., HOLT S.S., MUSHOTZKY R.F., PRAVDO S.H., ROTHSCHILD R.E., SERLEMITSOS P.J. Astrophys. J., Suppl. Ser., 40, 657-666 (1979) New hard X-ray sources observed with HEAO A-2. oTable 2: <H HHMM+DDd> N=47 Ref:=1983ApJS...51....1N byNUGENT J.J. , JENSEN K.A., NOUSEK J.A., GARMIRE G.P., MASON K.O., WALTER F.M., BOWYER C.S., STERN R.A., RIEGLER G.R. Astrophys. J., Suppl. Ser., 51, 1-28 (1983) HEAO A-2 soft X-ray source catalog. oTable 1: <H HHMM+DD> N=124
Details on Acronym: H
H (HEAO satellite)= (H4) = (HEAO) = (HEAO 4-) Write:<<H HHMM+DDd>> N: 72 Object:(Hard X) (SIMBAD class: X = X-ray Source) Note:All sky. 4 channels in the 13-180keV range. Observations from 1977 August to 1979 January. Data obtained with the UCSD/MIT Hard X-ray and Low-Energy X-ray Instrument on the HEAO 1 satellite. The survey is complete down to an intensity level 1/75 of the Crab Nebulae in the 13-80 keV energy band. 44 sources detected in the 40-80 keV energy band. 7 sources are extragalactic. Ref:=1984ApJS...54..581L byLEVINE A.M. , LANG F.L., LEWIN W.H.G., PRIMINI F.A., DOBSON C.A., DOTY J.P., HOFFMAN J.A., HOWE S.K., SCHEEPMAKER A., WHEATON W.A., MATTESON J.L., BAITY W.A., GRUBER D.E., KNIGHT F.K., NOLAN P.L., PELLING R.M., ROTHSCHILD R.E., PETERSON L.E. Astrophys. J., Suppl. Ser., 54, 581-617 (1984) The HEAO1 A-4 catalog of high-energy X-ray sources. oTable 5: <H HHMM+DDd> N=72
Details on Acronym: H
H (Hubble) ***** Avoid the usage of H, prefer [H29] Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (Hubble) ***** Avoid the usage of H, prefer [H32] Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (Hoffleit) ***** Avoid the usage of H, prefer [H53] Originof the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: H
H (Hodge) ***** Avoid the usage of H, prefer [H60b]
Details on Acronym: H
H (Hodge) ***** Avoid the usage of H, prefer [H65] Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (cloud complex labelled H) ***** Avoid the usage of H, prefer [H68] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H (Hodge) ***** Avoid the usage of H, prefer [H74b] Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (Hodge) ***** Avoid the usage of H, prefer [H76] Originof the Acronym: L (1999ApJ...510..104B)
Details on Acronym: H
H (Hodge) ***** Avoid the usage of H, prefer [H77] Originof the Acronym: L (1980A&AS...40...67D)
Details on Acronym: H
H (Hawkins) ***** Avoid the usage of H, prefer [H83] Originof the Acronym: L (Veron)
Details on Acronym: H
H (Hubble Deep Field) ***** Avoid the usage of H, prefer [HCB98] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H (Hickson) ***** Avoid the usage of H, prefer HCG Originof the Acronym: L (1993ApJS...85....1N)
Details on Acronym: H
H (Holtzman+) ***** Avoid the usage of H, prefer [HFS92] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H
H (Hazard+) ***** Avoid the usage of H, prefer [HMT84] Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (Hoglund) ***** Avoid the usage of H, prefer NRAO
Details on Acronym: H
H (Haddock) ***** Avoid the usage of H, prefer NRL
Details on Acronym: H
H (Haro)= H 1- = (Haro 2-). H 2- = (Haro 3-). H 3- = (Haro 6-) Write:<<PN H 1-NN>>
<<PN H 2-NN>>
<<PN H 3-NN>>
<<PN H 4-N>> N: 67+48+2+1 Object:PN + Poss. PN (SIMBAD class: PlanetaryNeb = Planetary Nebula) Stat:is completely incorporated in Simbad Note:List 1: format '1-NN', table 1 in ref. 1952BOTT....1a...1H, H 1-25 and H 1-49 are rejected as PN in 1992, Acker+ catalog.
List 2: format '2-NN', table 2 in ref. 1952BOTT....1a...1H, H 2-9 is a Nova.
List 3: format '3-NN', two objects in ref. 1953BOTT....1h...3H are PN
List4: format '4-N', in ref. 1951PASP...63..144H Ref:=1952BOTT....1a...1H byHARO G. Bol. Obs. Tonantz. Tacub., 1, part no 1, 1-None (1952) Nuevas nebulosas planetarias y objetos con emision en la region del centro galactico. oTable I: <PN H 1-NN> (Nos 1-1 to 1-67). Table II: <PN H 2-NN> (Nos 2-1 to 2-48). Ref:=1951PASP...63..144H byHARO G. Publ. Astron. Soc. Pac., 63, 144-145 (1951) Emission object in Coma. oPN H 4-1 = PK 049+88 1 o<PN H 4-N> (No. 4-1). Ref:=1953BOTT....1h...3H byHARO G. , IRIARTE B., CHAVIRA E. Bol. Obs. Tonantz. Tacub., 1, part no 8, 3-18 (1953) Nuevas estrellas con emission en las regiones obscuras del Toro-Auriga-Orion investigadas por Joy. oHaro 6-29 = PN H 3-29, Haro 6-75 = PN H 3-75. o<Haro 6-NN> (Nos 6-1 to 6-75). <PN H 3-NN> N=2 (Nos 3-29, 3-75).
Details on Acronym: H
H (Hoffleit) ***** Avoid the usage of H, prefer Hf
Details on Acronym: H
H (HI Hole) ***** Avoid the usage of H, prefer [PWB92] Originof the Acronym: L (1999AJ....118..323R)
Details on Acronym: H
H (HRI obs.) ***** Avoid the usage of H, prefer [SBF2000] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H (Harris) ====>Equivalent to: [SRB2011] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H (Hubble) ***** Avoid the usage of H, prefer [V62] Originof the Acronym: L = Found in the literature
Details on Acronym: H
H (HST) ***** Avoid the usage of H, prefer [VFK98] Originof the Acronym: L (2007ApJ...661..750T)
Details on Acronym: H
H (Hubble) ***** Avoid the usage of H, prefer VHK Originof the Acronym: L = Found in the literature
Details on Acronym: H4
H4 (HEAO satellite, 4th experience) ***** Avoid the usage of H4, prefer H
Details on Acronym: Haro 2-
Haro 2- (Haro, list 2) Note:List Haro 2- is synonyme of PN H 1-NN (N=67) ***** Avoid the usage of Haro 2-, prefer H
Details on Acronym: Haro 3-
Haro 3- (Haro, list 3) Note:List Haro 3- is synonyme of PN H 2-NN (N=48) ***** Avoid the usage of Haro 3-, prefer H
Details on Acronym: HEAO
HEAO (HEAO satellite) ***** Avoid the usage of HEAO, prefer H
Details on Acronym: HEAO 4-
HEAO 4- (HEAO satellite, 4th experience) ***** Avoid the usage of HEAO 4-, prefer H
Details on Acronym: Lick H
Lick H (Lick obs., H-alpha) ***** Avoid the usage of Lick H, prefer LkHA
Details on Acronym: OH
OH (Ohio univ., H stands for 7th hour of RA) ====>Equivalent to: Ohio Originof the Acronym: L = Found in the literature
Details on Acronym: Cl* AM 1 H
Cl* AM 1 H (Hilker) Write:<<Cl* AM 1 H NNN>> N: 160 Object:*inCl Ref:=2006A&A...448..171H byHILKER M. Astron. Astrophys., 448, 171-180 (2006) Probable member stars of the gravitational theory-testing globular clusters AM 1, Pal 3 and Pal 14. oTable A1: <Cl* AM 1 H NNN> (Nos 1-160). Table A2: <Cl* Palomar 3 H NNN> (Nos 1-153). Table A3: <Cl* Palomar 14 H NNN> (Nos 1-143). =E=Catalogue in electronic form as <J/A+A/448/171/>
Details on Acronym: Cl* Basel 12 H
Cl* Basel 12 H (Hassan) Write:<<Cl* Basel 12 H NN>> N: 75 Object:*inCl Ref:=1975A&AS...20..255H byHASSAN S.M. Astron. Astrophys., Suppl. Ser., 20, 255-267 (1975) The stellar groups Ba12, Ba13, Ba14 and Ba15. oTable 1: <Cl* Basel 12 H NN> (Nos 1-75), <Cl* Basel 13 H NNN> N=77 among (Nos 1-100), <Cl* Basel 14 H NNN> (Nos 1-107), <Cl* Basel 15 H NNN> (Nos 1-117).
Details on Acronym: Cl* Basel 13 H
Cl* Basel 13 H (Hassan) Write:<<Cl* Basel 13 H NNN>> N: 77 Object:*inCl Ref:=1975A&AS...20..255H byHASSAN S.M. Astron. Astrophys., Suppl. Ser., 20, 255-267 (1975) The stellar groups Ba12, Ba13, Ba14 and Ba15. oTable 1: <Cl* Basel 12 H NN> (Nos 1-75), <Cl* Basel 13 H NNN> N=77 among (Nos 1-100), <Cl* Basel 14 H NNN> (Nos 1-107), <Cl* Basel 15 H NNN> (Nos 1-117).
Details on Acronym: Cl* Basel 14 H
Cl* Basel 14 H (Hassan) Write:<<Cl* Basel 14 H NNN>> N: 107 Object:*inCl Ref:=1975A&AS...20..255H byHASSAN S.M. Astron. Astrophys., Suppl. Ser., 20, 255-267 (1975) The stellar groups Ba12, Ba13, Ba14 and Ba15. oTable 1: <Cl* Basel 12 H NN> (Nos 1-75), <Cl* Basel 13 H NNN> N=77 among (Nos 1-100), <Cl* Basel 14 H NNN> (Nos 1-107), <Cl* Basel 15 H NNN> (Nos 1-117).
Details on Acronym: Cl* Basel 15 H
Cl* Basel 15 H (Hassan) Write:<<Cl* Basel 15 H NNN>> N: 117 Object:*inCl Ref:=1975A&AS...20..255H byHASSAN S.M. Astron. Astrophys., Suppl. Ser., 20, 255-267 (1975) The stellar groups Ba12, Ba13, Ba14 and Ba15. oTable 1: <Cl* Basel 12 H NN> (Nos 1-75), <Cl* Basel 13 H NNN> N=77 among (Nos 1-100), <Cl* Basel 14 H NNN> (Nos 1-107), <Cl* Basel 15 H NNN> (Nos 1-117).
Details on Acronym: Cl* Hogg 18 H
Cl* Hogg 18 H (Hogg) ====>Equivalent to: Cl Hogg 18
Details on Acronym: Cl* Hogg 18 H
Cl* Hogg 18 H Write:<<Cl* Hogg 18 H a>> N: 18 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1961Obs....81...69H byHOGG A.R. The Observatory, 81, 69-76 (1961) A southern galactic cluster. oTable I: <Cl Hogg 18 NN> (Nos 1-16). Table II: <Cl* Hogg 18 H a> (Nos a-t).
Details on Acronym: Cl* IC 1369 H
Cl* IC 1369 H (Hassan) ====>Equivalent to: IC 1369
Details on Acronym: Cl* IC 2391 H
Cl* IC 2391 H (Hogg) Write:<<Cl* IC 2391 H NN>> N: 39 Object:*inCl Ref:=1960PASP...72...85H byHOGG A.R. Publ. Astron. Soc. Pac., 72, 85-93 (1960) The galactic cluster IC 2391. oTable I: <Cl* IC 2391 H NN> (Nos 0-38)
Details on Acronym: Cl* IC 348 H
Cl* IC 348 H (Herbig) Write:<<Cl* IC 348 H NNN>> N: 261 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1998ApJ...497..736H byHERBIG G.H. Astrophys. J., 497, 736-758 (1998) The young cluster IC 348. oTable 1: <Cl* IC 348 H NNN> (Nos 1-261). Tables 1, 6: <IfAHA NNN> (Nos 59-102). =E=Catalogue in electronic form as <J/ApJ/497/736/>
Details on Acronym: Cl* IC 348 IfA
Cl* IC 348 IfA (Institute for Astron. in Hawaii) ====>Equivalent to: Cl* IC 348 H
Details on Acronym: Cl* King 10 H
Cl* King 10 H (Handschel) Write:<<Cl* King 10 H NN>> N: 70 Object:*inCl Ref:=1972Thesi........0H byHANDSCHEL G. , -1-None (1972) UBV-Photometrie der offenen Sternhaufen NGC 7419, K 10 und NGC 6192. o<NGC 7419 NNN> Nos among (Nos 1-105), <NGC 6192 NNN> Nos among (Nos 1-108), <Cl* King 10 H NN> Nos among (Nos 1-70).
Details on Acronym: Cl* King 14 H
Cl* King 14 H (Hardorp) ====>Equivalent to: Cl King 14
Details on Acronym: Cl* Melotte 22 H
Cl* Melotte 22 H (Hertzprung) ====>Equivalent to: Cl Melotte 22
Details on Acronym: Cl* Melotte 25 H
Cl* Melotte 25 H (Hyades) ====>Equivalent to: Cl* Melotte 25 DKJ
Details on Acronym: Cl* Melotte 25 H
Cl* Melotte 25 H (Hanson) ====>Equivalent to: Cl* Melotte 25 Han
Details on Acronym: Cl* NGC 103 H
Cl* NGC 103 H (Hardorp) ====>Equivalent to: NGC 103
Details on Acronym: Cl* NGC 1647 H
Cl* NGC 1647 H (Hertzsprung) Write:<<Cl* NGC 1647 H NNN>> N: 219 Object:*inCl Ref:=1915ApJ....42...92H byHERTZSPRUNG E. Astrophys. J., 42, 92-110 (1915) Effective wavelengths of 184 stars in the cluster NGC 1647. o<Cl* NGC 1647 H NNN> (Nos 1-219).
Details on Acronym: Cl* NGC 1844 H
Cl* NGC 1844 H (Hodge) Write:<<Cl* NGC 1844 H NN>> N: 27 Object:*inCl Ref:=1961ApJ...134..226H byHODGE P.W. Astrophys. J., 134, 226-231 (1961) Studies of the Large Magellanic Cloud. VII. The open cluster NGC 1844. oTable I: <Cl* NGC 1844 H NN> (Nos 1-27).
Details on Acronym: Cl* NGC 1893 H
Cl* NGC 1893 H (Hovhannessian) Write:<<Cl* NGC 1893 H NNN>> N: 255 O *inCl Ref:=2007Ap.....50..194H byHOVHANNESSIAN R.K. Ap, 50, 194-202 (2007) Distribution of Early-Type Stars and Dusty Matter in the Direction of the Stellar Cluster NGC 1893. oTable 2: <[H2007b] Group R> (Nos I-XVI). Table 1, col(2): <Cl* NGC 1893 H NNN> (Nos 1-255). =E=Catalogue in electronic form as <J/other/Ap/50.194/>
Details on Acronym: Cl* NGC 2175 H
Cl* NGC 2175 H (Haikala) Write:<<Cl* NGC 2175 H NNN>> N: 169 Object:*inCl Ref:=1994A&AS..108..643H byHAIKALA L.K. Astron. Astrophys., Suppl. Ser., 108, 643-651 (1994) UBVRI photometry and polarimetry of the stars in S 252 (NGC 2175). I. The observations. oLS DD NN = LS V +DD NN o<Cl* NGC 2175 H NNN> N=169
Details on Acronym: Cl* NGC 2204 H
Cl* NGC 2204 H (Hawarden) ====>Equivalent to: NGC 2204
Details on Acronym: Cl* NGC 2243 H
Cl* NGC 2243 H (Hawarden) ====>Equivalent to: NGC 2243
Details on Acronym: Cl* NGC 2423 H
Cl* NGC 2423 H (Hassan) ====>Equivalent to: NGC 2423
Details on Acronym: Cl* NGC 2682 H
Cl* NGC 2682 H (Hoag) Write:<<Cl* NGC 2682 H NN>> N: 11 Object:*inCl Ref:=1976PASP...88..860H byHOAG A.A. Publ. Astron. Soc. Pac., 88, 860-864 (1976) Faint blue objects in the field of M 67. oTable I: <Cl* NGC 2682 H NN> (Nos 1-11).
Details on Acronym: Cl* NGC 2682 H
Cl* NGC 2682 H (Herstmonceux) ====>Equivalent to: Cl* NGC 2682 MC
Details on Acronym: Cl* NGC 3228 H
Cl* NGC 3228 H (Hogg) ====>Equivalent to: NGC 3228
Details on Acronym: Cl* NGC 3603 H
Cl* NGC 3603 H (HST telescope) ====>Equivalent to: Cl* NGC 3603 MDS Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: Cl* NGC 5617 H
Cl* NGC 5617 H (Haug) ====>Equivalent to: NGC 5617
Details on Acronym: Cl* NGC 5662 H
Cl* NGC 5662 H (Haug) ====>Equivalent to: NGC 5662
Details on Acronym: Cl* NGC 6025 H
Cl* NGC 6025 H (Hogg) ====>Equivalent to: Cl* NGC 6025 Wood
Details on Acronym: Cl* NGC 6139 H
Cl* NGC 6139 H (Hazen-Liller) Write:<<Cl* NGC 6139 H A>> N: 10 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6167 H
Cl* NGC 6167 H (Haffner) ====>Equivalent to: Cl* NGC 6167 BS
Details on Acronym: Cl* NGC 6192 H
Cl* NGC 6192 H (Handschel) ====>Equivalent to: NGC 6192
Details on Acronym: Cl* NGC 6259 H
Cl* NGC 6259 H (Hawarden) ====>Equivalent to: NGC 6259
Details on Acronym: Cl* NGC 6304 H
Cl* NGC 6304 H (Hesser) Write:<<Cl* NGC 6304 H NN>> N: 25 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1976PASP...88..849H byHESSER J.E. Publ. Astron. Soc. Pac., 88, 849-859 (1976) The interstellar reddening in the direction of four low-latitude globular clusters. oT.V: PG = Cl* NGC 6656 PG NN, P A are from Philp, 1974, private communication. oTable I: <Cl* NGC 6304 H NN> (Nos 1-25). Table II: <Cl* NGC 6352 H NN> (Nos 1-22). Table IV: <Cl* NGC 6441 H NN> (Nos 1-14). Table V: <Cl* NGC 6656 P A> (Nos A, C), <Cl* NGC 6656 H NN> (Nos 40, 43, 46).
Details on Acronym: Cl* NGC 6352 H
Cl* NGC 6352 H (Hesser) Write:<<Cl* NGC 6352 H NN>> N: 22 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1976PASP...88..849H byHESSER J.E. Publ. Astron. Soc. Pac., 88, 849-859 (1976) The interstellar reddening in the direction of four low-latitude globular clusters. oT.V: PG = Cl* NGC 6656 PG NN, P A are from Philp, 1974, private communication. oTable I: <Cl* NGC 6304 H NN> (Nos 1-25). Table II: <Cl* NGC 6352 H NN> (Nos 1-22). Table IV: <Cl* NGC 6441 H NN> (Nos 1-14). Table V: <Cl* NGC 6656 P A> (Nos A, C), <Cl* NGC 6656 H NN> (Nos 40, 43, 46).
Details on Acronym: Cl* NGC 6355 H
Cl* NGC 6355 H (Hazen-Liller) Write:<<Cl* NGC 6355 H A>> N: 10 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6441 H
Cl* NGC 6441 H (Hesser) Write:<<Cl* NGC 6441 H NN>> N: 14 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1976PASP...88..849H byHESSER J.E. Publ. Astron. Soc. Pac., 88, 849-859 (1976) The interstellar reddening in the direction of four low-latitude globular clusters. oT.V: PG = Cl* NGC 6656 PG NN, P A are from Philp, 1974, private communication. oTable I: <Cl* NGC 6304 H NN> (Nos 1-25). Table II: <Cl* NGC 6352 H NN> (Nos 1-22). Table IV: <Cl* NGC 6441 H NN> (Nos 1-14). Table V: <Cl* NGC 6656 P A> (Nos A, C), <Cl* NGC 6656 H NN> (Nos 40, 43, 46).
Details on Acronym: Cl* NGC 6453 H
Cl* NGC 6453 H (Hazen-Liller) Write:<<Cl* NGC 6453 H A>> N: 10 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6496 H
Cl* NGC 6496 H (Hazen-Liller) Write:<<Cl* NGC 6496 H A>> N: 8 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6558 H
Cl* NGC 6558 H (Hazen-Liller) Write:<<Cl* NGC 6558 H A>> N: 9 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6558 H
Cl* NGC 6558 H (Hazen) Write:<<Cl* NGC 6558 H a>>
<<Cl* NGC 6558 H FNN>> N: 14+46 Object:*inCl Rem:Table 2: secondary standards, (Nos a-q)
Table 5: 'Cl* NGC 6558 Saw VNN' continuation of 1973PDDO....3....6S
Table 6: field V*, (Nos F1-F46) Ref:=1996AJ....111.1184H byHAZEN M.L. Astron. J., 111, 1184-1192 (1996) A search for variable stars in the globular clusters NGC 5694 and NGC 6558. oTable 2: <Cl* NGC 6558 H a> (Nos a-q). Table 5: <Cl* NGC 6558 Saw VNN> (Nos V10-V15) added. Table 6: <Cl* NGC 6558 HFNN> (Nos F1-F46).
Details on Acronym: Cl* NGC 6569 H
Cl* NGC 6569 H (Hazen-Liller) Write:<<Cl* NGC 6569 H A>> N: 10 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6569 H
Cl* NGC 6569 H (Hazen-Liller) Write:<<Cl* NGC 6569 H VNN>>
<<Cl* NGC 6569 H FNN>> N: 23+22 Object:*inCl Rem:Table III: V* in NGC 6569, format 'VNN'.
Table VI: V* in the field around 6569, format 'FNN'. Ref:=1985AJ.....90.1807H byHAZEN-LILLER M.L. Astron. J., 90, 1807-1811 (1985) The variable stars in the field of the globular cluster NGC 6569. oTable III: <Cl* NGC 6569 H VNN> (Nos V1-V23). Table VI: <Cl* NGC 6569 H FNN> (Nos F1-F22).
Details on Acronym: Cl* NGC 6618 H
Cl* NGC 6618 H (Hoffmeister+)
Details on Acronym: Cl* NGC 6642 H
Cl* NGC 6642 H (Hazen-Liller) Write:<<Cl* NGC 6642 H A>> N: 11 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6652 H
Cl* NGC 6652 H (Hazen-Liller) Write:<<Cl* NGC 6652 H A>> N: 12 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6656 H
Cl* NGC 6656 H (Hesser) Write:<<Cl* NGC 6656 H NN>> N: 3 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1976PASP...88..849H byHESSER J.E. Publ. Astron. Soc. Pac., 88, 849-859 (1976) The interstellar reddening in the direction of four low-latitude globular clusters. oT.V: PG = Cl* NGC 6656 PG NN, P A are from Philp, 1974, private communication. oTable I: <Cl* NGC 6304 H NN> (Nos 1-25). Table II: <Cl* NGC 6352 H NN> (Nos 1-22). Table IV: <Cl* NGC 6441 H NN> (Nos 1-14). Table V: <Cl* NGC 6656 P A> (Nos A, C), <Cl* NGC 6656 H NN> (Nos 40, 43, 46).
Details on Acronym: Cl* NGC 6717 H
Cl* NGC 6717 H (Hazen-Liller) Write:<<Cl* NGC 6717 H A>> N: 10 Object:*inCl Ref:=1984AJ.....89.1551H byHAZEN-LILLER M.L. Astron. J., 89, 1551-1558 (1984) Photoelectric sequences near nine galactic globular clusters. oTable II: <Cl* NGC 6139 H A> (Nos A-J), <Cl* NGC 6355 H A> (Nos A-K, I missing), <Cl* NGC 6453 H A> (Nos A-J), <Cl* NGC 6496 H A> (Nos A-H), <Cl* NGC 6558 H A> N=9 among (Nos A-L), <Cl* NGC 6569 H A> (Nos A-K, I missing), <Cl* NGC 6642 H A> N=11 among (Nos A-P), <Cl* NGC 6652 H A> (Nos A-L), <Cl* NGC 6717 H A> (Nos A-J).
Details on Acronym: Cl* NGC 6838 H
Cl* NGC 6838 H (Hodder+) Write:<<Cl* NGC 6838 H NNNN>> N: 1861 Object:*inCl Ref:=1992AJ....103..460H byHODDER P.J.C. , NEMEC J.M., RICHER H.B., FAHLMAN G. Astron. J., 103, 460-479 (1992) Deep CCD photometry and variable stars in the metal-rich globular cluster M 71. oTable 2: <Cl* NGC 6838 H NNNN> (Nos 1-1861). =E=Catalogue in electronic form as <J/AJ/103/460/> Originof the Acronym: L (2000AJ....119.1803P)
Details on Acronym: Cl* NGC 6838 HNRF
Cl* NGC 6838 HNRF (Hodder+Nemec+Richer+Fahlman) ====>Equivalent to: Cl* NGC 6838 H
Details on Acronym: Cl* NGC 7039 H
Cl* NGC 7039 H (Hassan) ====>Equivalent to: NGC 7039
Details on Acronym: Cl* NGC 7067 H
Cl* NGC 7067 H (Hassan) Write:<<Cl* NGC 7067 H NNN>> N: 111 Object:*inCl Ref:=1973A&AS....9..261H byHASSAN S.M. Astron. Astrophys., Suppl. Ser., 9, 261-287 (1973) Three colour photometry of the five open clusters NGC 7039, NGC 7062, NGC 7067, NGC 7082, IC 1369. oTable 5: stars are Cl* NGC 7062 F NNN in SIMBAD. oTable 2: <NGC 7082 NNN> (Nos 1-200). Table 3: <IC 1369 NNN> (Nos 1-183). Table 4: <NGC 7039 NNN> (Nos 1-204). Table 6a: <Cl* NGC 7067 H NNN> (Nos 1-111).
Details on Acronym: Cl* NGC 7082 H
Cl* NGC 7082 H (Hassan) ====>Equivalent to: NGC 7082
Details on Acronym: Cl* NGC 7086 H
Cl* NGC 7086 H (Hassan) ====>Equivalent to: NGC 7086
Details on Acronym: Cl* NGC 7086 H
Cl* NGC 7086 H (Hassan) ====>Equivalent to: Cl* NGC 7086 Has
Details on Acronym: Cl* NGC 7086 H
Cl* NGC 7086 H (Hoag) ====>Equivalent to: Cl* NGC 7086 Hoag
Details on Acronym: Cl* NGC 7419 H
Cl* NGC 7419 H (Handschel) ====>Equivalent to: NGC 7419
Details on Acronym: Cl* NGC 752 H
Cl* NGC 752 H (Heinemann) ====>Equivalent to: NGC 752
Details on Acronym: Cl* Palomar 14 H
Cl* Palomar 14 H (Hilker) Write:<<Cl* Palomar 14 H NNN>> N: 143 Object:*inCl Ref:=2006A&A...448..171H byHILKER M. Astron. Astrophys., 448, 171-180 (2006) Probable member stars of the gravitational theory-testing globular clusters AM 1, Pal 3 and Pal 14. oTable A1: <Cl* AM 1 H NNN> (Nos 1-160). Table A2: <Cl* Palomar 3 H NNN> (Nos 1-153). Table A3: <Cl* Palomar 14 H NNN> (Nos 1-143). =E=Catalogue in electronic form as <J/A+A/448/171/> Historyof this Acronym: replaces Cl* Palomar 4 H
Details on Acronym: Cl* Palomar 3 H
Cl* Palomar 3 H (Hilker) Write:<<Cl* Palomar 3 H NNN>> N: 153 Object:*inCl Ref:=2006A&A...448..171H byHILKER M. Astron. Astrophys., 448, 171-180 (2006) Probable member stars of the gravitational theory-testing globular clusters AM 1, Pal 3 and Pal 14. oTable A1: <Cl* AM 1 H NNN> (Nos 1-160). Table A2: <Cl* Palomar 3 H NNN> (Nos 1-153). Table A3: <Cl* Palomar 14 H NNN> (Nos 1-143). =E=Catalogue in electronic form as <J/A+A/448/171/>
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