CDS

Dictionary of Nomenclature of Celestial Objects
(Last update: 02-Jun-2023)

Result of query: info cati PM JHHMMm+DDMMWw$ 



.
 


Details on Acronym:   OPM
  
OPM    (Ohio univ., P stands for 14th hour of RA, M stands for Medium-Velocity)
  ***** Avoid the usage of OPM,  prefer Ohio
 Originof the Acronym: L = Found in the literature

Details on Acronym:   PM
  
PM     (Proper Motion)= (PMI) = (PMII) = (PMIII) 
 Write:<<PM  HHMMm+DDMMA>>  

        <<PM  JHHMMm+DDMM>>  

        <<PM  JHHMMm+DDMMW>>  

        <<PM  JHHMMm+DDMMWw>>

<<PM  IHHMMm+DDMM>>	(not recognised by Simbad, but found in literature)
Object:PM*  (SIMBAD class: HighPM* = High Proper Motion Star)
  Note:Format HHMMm+DDMMA: Catalogs of proper motion stars published    by Eggen (the first two references given here).
    Format JHHMMm+DDMMW: Proper motion stars in the SUPERBLINK    proper motion survey, following the convention introduced by    Eggen. See also LSR.
   Ref:=1979ApJS...39...89E
     byEGGEN O.J.

 Astrophys. J., Suppl. Ser., 39, 89-101 (1979)

    Catalogs of proper-motion stars. I. Stars brighter than visual
    magnitude 15 and with annual proper motion of 1" or more.
oTable 1A: <PM HHMMm+DDMMA> N=430
   Ref:=1980ApJS...43..457E
     byEGGEN O.J.

 Astrophys. J., Suppl. Ser., 43, 457-468 (1980)

    Catalogs of proper motion stars. II. Stars brighter than visual
    magnitude 15 and south of declination +30 with annual proper motion    between 0"7 and 1"0.
oCorrection in EGGEN O.J., 1983, Ap.J.Suppl. 51, 183-202
oTable 1: <PM HHMMm+DDMMA> N=434
   Ref:=2005AJ....130.1247L
     byLEPINE S.

 Astron. J., 130, 1247-1260 (2005)

    New high proper motion stars from the Digitized Sky Survey. III. Stars with
    proper motions 0.45"<µ<2.0"/yr south of  declination -30°.
oTable 1: <PM JHHMMm+DDMMW> N=182.
   Ref:=2008AJ....135.2177L
     byLEPINE S.

 Astron. J., 135, 2177-2193 (2008)

    New high proper motion stars from the Digitized Sky Survey. IV. Completion
    of the southern survey and 170 additional stars with µ>0.45"/yr.
oTable 1: <PM JHHMMm+DDMMW> N=170 added.
   Ref:=2010AJ....140..119S
     bySCHLIEDER J.E.
, LEPINE S., SIMON M.
 Astron. J., 140, 119-128 (2010)

    β Pictoris and AB Doradus moving groups: likely new low-mass members.

oTable 1: <PM JHHMMm+DDMMW> N=8 added.
   Ref:=2011AJ....142..138L
     byLEPINE S.
, GAIDOS E.
 Astron. J., 142, 138 (2011)

    An all-sky catalog of bright M dwarfs.

oTables 1-2: <PM JHHMMm+DDMMW> N=8889.
   Ref:=2012AJ....143...80S
     bySCHLIEDER J.E.
, LEPINE S., SIMON M.
 Astron. J., 143, 80 (2012)

    Cool young stars in the northern hemisphere: β Pictoris and AB  Doradus
    moving group candidates.
oTables 1, 3: <PM JHHMMm+DDMMW> N=6+7 added. Table 2: <[SLS2012] PYC    JHHMMm+DDMMW> N=204.
   Ref:=2013AJ....145..102L
     byLEPINE S.
, HILTON E.J., MANN A.W., WILDE M., ROJAS-AYALA B., CRUZ K.L., GAIDOS E.
 Astron. J., 145, 102 (2013)

    A spectroscopic catalog of the brightest (J<9) M dwarfs in the northern sky.

oTables 1, 3, 6-7: <PM JHHMMm+DDMMWw> N=1564.
=E=Catalogue in electronic form as <J/AJ/140/119/>
=E=Catalogue in electronic form as <J/AJ/143/80/>
=E=Catalogue in electronic form as J/AJ/142/138
=E=Catalogue in electronic form as <J/AJ/145/102/>
 Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   PM
  
PM     (Proper Motion)
 Write:<<PM  JHHMMm+DDMMA>>  

        <<PM  JHHMMm+DDMMW A>>  

        <<PM  JHHMMm+DDMMWw A>>
Object:PM*  (SIMBAD class: HighPM* = High Proper Motion Star)
  Note:Suffix A added to follow in SIMBAD the usage found in the literature    regarding multiple star systems.
    It is an extension of the convention introduced by Eggen for proper    motion stars.
 Originof the Acronym: L = Found in the literature

Details on Acronym:   PM
  
PM     (Parker+Morgan+)
  ***** Avoid the usage of PM,  prefer PMR
 Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   PM
  
PM     (Preite-Martinez)
 Write:<<PN PM  1-NNN>>  

        <<PN PM  2-NN>>
 N:  340+48
Object:Poss. PN  (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
  Note:Table IV: PM 1-, list 1, N=340,    sources with a high probability of being a PN
    Table V: PM 2-, list 2, N=48,    sources with a high probability of being non-PN,    or only PN-related objects.
   Ref:=1988A&AS...76..317P
     byPREITE-MARTINEZ A.

 Astron. Astrophys., Suppl. Ser., 76, 317-330 (1988)

    Possible new planetary nebulae in the IRAS point source catalogue.

oTables IV and V list Planetary Nebula Candidates selected on IRAS colours. The    historical choice of the acronym PN PM , where PN means confirmed Planetary    Nebula, was thus not correct. This acronym PN PM has been kept only on confirmed    PNe (83 in January 2023). A new acronym [P88b] PM N-NNN is going to be created    in SIMBAD, with a default object type PN?. Until it is ready, please use the    IRAS identifier.
oTable IV: <[P88b] PM 1-NNN> (Nos 1-340) = <PN PM 1-NNN> (Nos 1-340). Table V:    <[P88b] PM 2-NN> (Nos 1-48) = <PN PM 2-NN> (Nos 1-48).
=E=Catalogue in electronic form as <J/A+AS/76/317/>
 Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   PMI
  
PMI    (Proper motion, I: (roman num.) 1st catalog)
  ***** Avoid the usage of PMI,  prefer PM

Details on Acronym:   PMII
  
PMII   (Proper motion, II: (roman num.) 2nd catalog)
  ***** Avoid the usage of PMII,  prefer PM

Details on Acronym:   PMIII
  
PMIII  (Proper motion, III: (roman num.) 3rd catalog)
  ***** Avoid the usage of PMIII,  prefer PM

Details on Acronym:   Cl* NGC 2439 PM
  
Cl* NGC 2439 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 2439 PM  NNN>>
 N:  113
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2002A&A...385..867P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 385, 867-873 (2002)

    CCD photometric search for peculiar stars in open clusters. III. NGC
    2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451.
oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM    NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7:    <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos    1-146).
=E=Catalogue in electronic form as <J/A+A/385/867/>

Details on Acronym:   Cl* NGC 2489 PM
  
Cl* NGC 2489 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 2489 PM  NN>>
 N:  59
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2001A&A...373..153P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 373, 153-158 (2001)

    CCD photometric search for peculiar stars in open clusters. II. NGC
    2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208.
oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM    NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl*    NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).

Details on Acronym:   Cl* NGC 2567 PM
  
Cl* NGC 2567 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 2567 PM  NN>>
 N:  50
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2001A&A...373..153P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 373, 153-158 (2001)

    CCD photometric search for peculiar stars in open clusters. II. NGC
    2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208.
oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM    NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl*    NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).

Details on Acronym:   Cl* NGC 2658 PM
  
Cl* NGC 2658 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 2658 PM  NN>>
 N:  55
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2001A&A...373..153P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 373, 153-158 (2001)

    CCD photometric search for peculiar stars in open clusters. II. NGC
    2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208.
oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM    NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl*    NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).

Details on Acronym:   Cl* NGC 3960 PM
  
Cl* NGC 3960 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 3960 PM  NN>>
 N:  93
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2002A&A...385..867P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 385, 867-873 (2002)

    CCD photometric search for peculiar stars in open clusters. III. NGC
    2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451.
oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM    NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7:    <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos    1-146).
=E=Catalogue in electronic form as <J/A+A/385/867/>

Details on Acronym:   Cl* NGC 5281 PM
  
Cl* NGC 5281 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 5281 PM  NN>>
 N:  30
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2001A&A...373..153P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 373, 153-158 (2001)

    CCD photometric search for peculiar stars in open clusters. II. NGC
    2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208.
oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM    NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl*    NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).

Details on Acronym:   Cl* NGC 6134 PM
  
Cl* NGC 6134 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 6134 PM  NNN>>
 N:  102
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2002A&A...385..867P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 385, 867-873 (2002)

    CCD photometric search for peculiar stars in open clusters. III. NGC
    2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451.
oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM    NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7:    <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos    1-146).
=E=Catalogue in electronic form as <J/A+A/385/867/>

Details on Acronym:   Cl* NGC 6192 PM
  
Cl* NGC 6192 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 6192 PM  NN>>
 N:  98
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2002A&A...385..867P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 385, 867-873 (2002)

    CCD photometric search for peculiar stars in open clusters. III. NGC
    2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451.
oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM    NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7:    <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos    1-146).
=E=Catalogue in electronic form as <J/A+A/385/867/>

Details on Acronym:   Cl* NGC 6208 PM
  
Cl* NGC 6208 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 6208 PM  NN>>
 N:  41
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2001A&A...373..153P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 373, 153-158 (2001)

    CCD photometric search for peculiar stars in open clusters. II. NGC
    2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208.
oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM    NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl*    NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).

Details on Acronym:   Cl* NGC 6451 PM
  
Cl* NGC 6451 PM (Paunzen+Maitzen)
 Write:<<Cl* NGC 6451 PM  NNN>>
 N:  146
Object:*inCl
  Stat:is completely incorporated in Simbad
   Ref:=2002A&A...385..867P
     byPAUNZEN E.
, MAITZEN H.M.
 Astron. Astrophys., 385, 867-873 (2002)

    CCD photometric search for peculiar stars in open clusters. III. NGC
    2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451.
oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM    NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7:    <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos    1-146).
=E=Catalogue in electronic form as <J/A+A/385/867/>













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