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

Result of query: info cati SK$

Details on Acronym:   NS
   NS (N. Sanduleak) ***** Avoid the usage of NS, prefer Sk
Details on Acronym:   S
   S (Sanduleak) ***** Avoid the usage of S, prefer Sk Originof the Acronym: L (1968AJ.....73..246S)
Details on Acronym:   S
   S (Sanduleak) Note:1970CoTol..89....1S in the LMC: ***** Avoid the usage of S, prefer Sk
Details on Acronym:   Sa
   Sa (Sanduleak) ***** Avoid the usage of Sa, prefer Sk
Details on Acronym:   Sa
   Sa (Sanduleak) ***** Avoid the usage of Sa, prefer Sk Originof the Acronym: L = Found in the literature
Details on Acronym:   Sanduleak
   Sanduleak (Sanduleak) ***** Avoid the usage of Sanduleak, prefer Sk
Details on Acronym:   Sanduleak
   Sanduleak (Sanduleak) ***** Avoid the usage of Sanduleak, prefer Sk
Details on Acronym:   Sk
   Sk (Sanduleak)= (S) = (Sa) = (Sanduleak) Write:<<Sk NNN>> N: 216 Object:*  (SIMBAD class: Star) Stat:is completely incorporated in Simbad Note:Identif. charts. in source:Magellanic Clouds:SMC = SMC Ref:=1968AJ.....73..246S bySANDULEAK N. Astron. J., 73, 246-250 (1968) A finding list of proven or probable Small Magellanic Cloud members. oTable I: <Sk NNN> (Nos 1-169) Ref:=1969AJ.....74..877S bySANDULEAK N. Astron. J., 74, 877-878 (1969) Proven and probable members in the Wing of the Small Magellanic Cloud. oTable I: <Sk NNN> (Nos 170-216)
Details on Acronym:   Sk
   Sk (Sanduleak)= (NS) = (S) = (Sa) = (Sanduleak) Write:<<Sk -DD NNNa>> N: 1272 Object:*  (SIMBAD class: Star) Note:Sometimes found in the literature with formats 'NNN-DD' or '-DD/NNN' to avoid. ('NNN-DD' had been first introduced to make a clear discrimination from CPD then constantly used.)
Identif. charts in source:Magellanic Clouds:LMC = LMC Ref:=1970CoTol..89....1S bySANDULEAK N. Contr. Cerro-Tololo Obs., 89, 1-None (1970) A deep objective-prism survey for Large Magellanic Cloud members. oTable III: <Sk -DD NNNA> N=1272 =E=Catalogue in electronic form as III/113 =E=Catalogue in electronic form as <III/113A/>
Details on Acronym:   SK
   SK (Sandell+Knee) ***** Avoid the usage of SK, prefer [SK2001] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   SK
   SK (Sandage+Katem) ***** Avoid the usage of SK, prefer [SK76] Originof the Acronym: L (2007ApJ...671.2028B)
Details on Acronym:   SK
   SK (Simard-Normandin+Kronberg) ***** Avoid the usage of SK, prefer [SK80] Originof the Acronym: L (1989ApJ...343..760R)
Details on Acronym:   Sk
   Sk (Sanduleak) ***** Avoid the usage of Sk, prefer SkKM Originof the Acronym: L = Found in the literature
Details on Acronym:   Cl* Melotte 22 S
   Cl* Melotte 22 S (Stauffer+) ====>Equivalent to: Cl* Melotte 22 SK Originof the Acronym: L (1998A&A...335..183Q)
Details on Acronym:   Cl* Melotte 22 SK
   Cl* Melotte 22 SK (Stauffer+Klemola+) Write:<<Cl* Melotte 22 SK NNN>> N: 284 Object:*inCl Ref:=1991AJ....101..980S bySTAUFFER J. , KLEMOLA A., PROSSER C., PROBST R. Astron. J., 101, 980-1007 (1991) The search for faint members of the Pleiades. I. A proper motion membership study of the Pleiades to Mv - 12.5. oTable 1: <Cl* Melotte 22 SK NNN> N=284 among (Nos 7-802). Table 2: <Cl* Melotte 22 KLEM NNN> N=15 among (Nos 6-354).
Details on Acronym:   Cl* Melotte 22 SKP
   Cl* Melotte 22 SKP (Stauffer+Klemola+Prosser+) ====>Equivalent to: Cl* Melotte 22 SK
Details on Acronym:   Cl* NGC 5272 SK
   Cl* NGC 5272 SK (Sandage+Katem) Write:<<Cl* NGC 5272 SK NNN>> N: 676 Object:*inCl Ref:=1982AJ.....87..537S bySANDAGE A. , KATEM B. Astron. J., 87, 537-554 (1982) On the intrinsic widths of the subgiant and horizontal branch sequences in the globular cluster M 3. oTable I, col.1: incomplete format: CL* NGC 5272 S R-R-NNN with the first roman numeral I for Serie I. oTable II: <CL* NGC 5272 SK NNN> (Nos 1-676).
Details on Acronym:   Cl* NGC 5897 SK
   Cl* NGC 5897 SK (Sandage+Katem) ====>Equivalent to: NGC 5897
Details on Acronym:   Cl* NGC 5897 SK
   Cl* NGC 5897 SK (Sandage+Katem) Write:<<Cl* NGC 5897 SK A>> N: 20 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1968ApJ...153..569S bySANDAGE A. , KATEM B. Astrophys. J., 153, 569-575 (1968) The color-magnitude diagram for the globular cluster NGC 5897. oTable 1: <Cl* NGC 5897 SK A> (Nos A-T). Table 2: <NGC 5897 NNN> N=254 among (Nos 1-366).
Details on Acronym:   Cl* NGC 6171 DR
   Cl* NGC 6171 DR (Dickens+Rolland) ====>Equivalent to: Cl* NGC 6171 SK
Details on Acronym:   Cl* NGC 6171 SK
   Cl* NGC 6171 SK Write:<<Cl* NGC 6171 SK NNNA>>
<<Cl* NGC 6171 SK A>>
<<Cl* NGC 6171 SK Aa>> N: 468+3+28 Object:*inCl Rem:1964ApJ...139.1088S: (Nos 1-282), (Nos A-Z, Aa, Ba)

1972MNRAS.160...37D: (Nos 283-468) and 61A, 61B, 254A added
1992AJ....103.1252C: Nos 267N and 267S Ref:=1964ApJ...139.1088S bySANDAGE A. , KATEM B. Astrophys. J., 139, 1088-1094 (1964) Three-color photometry of the metal-riche globular cluster NGC 6171. oTable 1: <Cl* NGC 6171 SK A>, <Cl* NGC 6171 SK Aa>, N=28. Table 2: <Cl* NGC 6171 SK NNN> (Nos 1-282) Ref:=1972MNRAS.160...37D byDICKENS R.J. , ROLLAND A. Mon. Not. R. Astron. Soc., 160, 37-62 (1972) UBV photometry of the metal rich globular cluster NGC 6171. oTable I: <Cl* NGC 6171 DR FNNN> (Nos F1-F214). Table II: <Cl* NGC 6171 SK NNNA> (Nos 283-468, 61A, 61B, 254A are new) Ref:=1992AJ....103.1252C byCUDWORTH K.M. , SMETANKA J.J., MAJEWSKI S.R. Astron. J., 103, 1252-1258 (1992) The globular cluster M107: membership and kinematics. oTable 3: <Cl* NGC 6171 Y NNN> N=115 among (Nos 91-408). Table 3: <Cl* NGC 6171 SK NNNW> (Nos 267N, 267S) ADDED.
Details on Acronym:   Cl* NGC 6341 SK
   Cl* NGC 6341 SK (Sandage+Katem) Write:<<Cl* NGC 6341 SK NNNNNA>> N: 375 Object:*inCl Rem:Tables 1, 3:
Format 'NNNNNA' (6 digits):
The first digit is a Roman digit for ring (III or IV),
Translated by '3' or '4'.

the second digit is a subdivision of the ring (ex. ring IV-2),
the letter at the end of the format is a sector of a
ring,

and the 3 last digits 'NNN' are the numbering of a star
in each sector.

ex. star 39 in IV-1-B = Cl* NGC 6341 SK 41039B. Ref:=1983AJ.....88.1146S bySANDAGE A. , KATEM B. Astron. J., 88, 1146-1158 (1983) On the intrinsic width and luminosity function of the M 92 main sequence. oTables 1, 3: <Cl* NGC 6341 SK NNNNNA> N about 375.
Details on Acronym:   Cl* NGC 6624 SK
   Cl* NGC 6624 SK (Sosin+King) Write:<<Cl* NGC 6624 SK NNNN # 4 digits>> N: 784 Object:*inCl Rem:Format 'NNNN' is always a 4 digits format,
first digit 1 in table 1,
first digit 3 in table 2. Ref:=1995AJ....109..639S bySOSIN C. , KING I.R. Astron. J., 109, 639-649 (1995) HST observations of the core of the globular cluster NGC 6624. oTables 2, 3 are presented in their complete form in the AAS CD-ROM Series, vol. 4, 1995 oTables 1, 2: <Cl* NGC 6624 SK NNNN> always 4 digits format, N=784 =E=Catalogue in electronic form as <J/AJ/109/639/>

© Université de Strasbourg/CNRS

    • Contact