Dictionary of Nomenclature of Celestial Objects
(Last update: 23-Oct-2020)

Result of query: info cati Bol NNN$



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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: GlCl = 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: GlCl = 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).

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