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

Result of query: info cati Bol$

Details on Acronym:   B
  
B      (Bologna obs.)
  ***** Avoid the usage of B,  prefer Bol
 Originof the Acronym: L (2007AJ....133.2764B)

Details on Acronym:   Ba87
  
Ba87   (Battistini+, 1987)
  ***** Avoid the usage of Ba87,  prefer Bol
 Originof the Acronym: L (2001A&A...373...63S)

Details on Acronym:   Bo
  
Bo     (Bologna obs.)
  ***** Avoid the usage of Bo,  prefer Bol
 Originof the Acronym: L = Found in the literature

Details on Acronym:   Bol
  
Bol    (Bologna obs.)= (B) = (Ba87) = (Bo) = (N) 
 Write:<<Bol  NNN>>
 N:  530
Object:GlCl  (SIMBAD class: GlobCluster = Globular Cluster)
  Stat:is completely incorporated in Simbad
  Note:Bologna observatory search for globular clusters in M 31.
 in source:M 31 = NGC 224
   Ref:=1980A&AS...42..357B
     byBATTISTINI P.
, BONOLI F., BRACCESI A., FUSI PECCI F., MALAGNINI M.L., MARANO B.
 Astron. Astrophys., Suppl. Ser., 42, 357-374 (1980)

    Search for (globular) clusters in M 31. I. Candidates in a 70'square
    field centered on M 31.
oFinding charts
oTable III: <Bol NNN> (Nos 1-288), Table V: <Bol DNNN> (Nos D1-D132)
   Ref:=1987A&AS...67..447B
     byBATTISTINI P.
, BONOLI F., BRACCESI A., FEDERICI L., FUSI PECCI F., MARANO B., BOERNGEN F.
 Astron. Astrophys., Suppl. Ser., 67, 447-482 (1987)

    Search for (globular) clusters in M 31. IV. Candidates in a 3x3° square
    field centered on M 31.
oTable IV, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
oTable IV, col(1): <C MMSSDDMMm> N=113. Tables IV, V: <Bol NNN> (Nos    289-513, Nos 334 and 359 missing). Table VI: <Bol DNNN> (Nos    D133-D350).
   Ref:=2005A&A...436..535G
     byGALLETI S.
, BELLAZZINI M., FEDERICI L., FUSI PECCI F.
 Astron. Astrophys., 436, 535-540 (2005)

    The outermost cluster of M31.

oParagr.3: <Bol NNN> (No. 514) added.
   Ref:=2006A&A...456..985G
     byGALLETI S.
, FEDERICI L., BELLAZZINI M., BUZZONI A., FUSI PECCI F.
 Astron. Astrophys., 456, 985-999 (2006)

    An updated survey of globular clusters in M 31. I. Classification and
    radial velocity for 76 candidate clusters.
oFig.10: <Bol NNN> (No. 515) added.
   Ref:=2007A&A...471..127G
     byGALLETI S.
, BELLAZZINI M., FEDERICI L., BUZZONI A., FUSI PECCI F.
 Astron. Astrophys., 471, 127-136 (2007)

    An updated survey of globular clusters in M 31. II. Newly discovered
    bright and remote clusters.
oTable m31rbc.dat: <RBC NNNN> N=1983 among (Nos 1-7737). Tables 3, B1, text: <Bol    NNN> (Nos 516-524) added.
   Ref:=2007A&A...476..193B
     byBECCARI G.
, BELLAZZINI M., CLEMENTINI G., FEDERICI L., FUSI PECCI F., GALLETI S., MONTEGRIFFO P., GIALLONGO E., RAGAZZONI R., GRAZIAN A., BARUFFOLO A., DE SANTIS C., DIOLAITI E., DI PAOLA A., FARINATO J., FONTANA A., GALLOZZI S., GASPARO F., GENTILE G., GREEN R., HILL J., KUHN O., MENCI N., PASIAN F., PEDICHINI F., SMAREGLIA R., SPEZIALI R., TESTA V., THOMPSON D., VERNET E., WAGNER R.M.
 Astron. Astrophys., 476, 193-198 (2007)

    A near-ultraviolet view of the inner region of M 31 with the large
    binocular telescope.
oTable 1: <Bol NNN> (Nos 525-530) added.
=E=Catalogue in electronic form as J/A+A/471/127
=E=Catalogue in electronic form as <V/143/>
 Originof the Acronym: L = Found in the literature

Details on Acronym:   Bol
  
Bol    (Bologna obs.)= (Bo) = (BolD) = (N) 
 Write:<<Bol  DNNN>>
 N:  350
Object:Misc. Obj.  (SIMBAD class: GlobCluster = Globular Cluster)
  Stat:is completely incorporated in Simbad
  Note:Table V in the first ref., Table VI in the second ref..    format 'DNNN': miscellaneous obj. of class D, not GCl.
 in source:M 31 = NGC 224
   Ref:=1980A&AS...42..357B
     byBATTISTINI P.
, BONOLI F., BRACCESI A., FUSI PECCI F., MALAGNINI M.L., MARANO B.
 Astron. Astrophys., Suppl. Ser., 42, 357-374 (1980)

    Search for (globular) clusters in M 31. I. Candidates in a 70'square
    field centered on M 31.
oFinding charts
oTable III: <Bol NNN> (Nos 1-288), Table V: <Bol DNNN> (Nos D1-D132)
   Ref:=1987A&AS...67..447B
     byBATTISTINI P.
, BONOLI F., BRACCESI A., FEDERICI L., FUSI PECCI F., MARANO B., BOERNGEN F.
 Astron. Astrophys., Suppl. Ser., 67, 447-482 (1987)

    Search for (globular) clusters in M 31. IV. Candidates in a 3x3° square
    field centered on M 31.
oTable IV, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
oTable IV, col(1): <C MMSSDDMMm> N=113. Tables IV, V: <Bol NNN> (Nos    289-513, Nos 334 and 359 missing). Table VI: <Bol DNNN> (Nos    D133-D350).
 Originof the Acronym: L = Found in the literature

Details on Acronym:   Bol
  
Bol    (Boller)
  ***** Avoid the usage of Bol,  prefer Boller
 Originof the Acronym: L (Veron)

Details on Acronym:   BolD
  
BolD   (Bologna obs., field D)
  ***** Avoid the usage of BolD,  prefer Bol
 Originof the Acronym: L = Found in the literature

Details on Acronym:   N
  
N      (Nebula)
  ***** Avoid the usage of N,  prefer Bol
 Originof the Acronym: L = Found in the literature

Details on Acronym:   Cl* NGC 288 Bol
  
Cl* NGC 288 Bol (Bolte)
 Write:<<Cl* NGC 288 Bol  NNN>>
 N:  982
Object:*inCl
   Ref:=1992ApJS...82..145B
     byBOLTE M.

 Astrophys. J., Suppl. Ser., 82, 145-165 (1992)

    CCD photometry in the globular cluster NGC 288. I. Blue stragglers and
    main-sequence binary stars.
oTable 5: <Cl* NGC 288 Bol NNN> (Nos 1-982), <Cl* NGC 288 BolBS NN>    (Nos 1-38), <Cl* NGC 288 BolB NN> (Nos 1-85).