Result of query: info cati
Sim NNN$
.
Details on Acronym: S
S (Simeis obs.)
Note:Ref. 1950S1: S 147, a wellknown galactic SNR, should be
***** Avoid the usage of S, prefer Sim
Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: S
S (Simeis obs.)
***** Avoid the usage of S, prefer Sim
Details on Acronym: SG
SG (Shajn+Gaze)
***** Avoid the usage of SG, prefer Sim
Details on Acronym: Sh
Sh (Shajn+)
***** Avoid the usage of Sh, prefer Sim
Details on Acronym: Shajn
Shajn (Shajn+)
***** Avoid the usage of Shajn, prefer Sim
Details on Acronym: SHZ
SHZ (Shajn+Gaze)
***** Avoid the usage of SHZ, prefer Sim
Details on Acronym: Si
Si (Simeis obs.)
***** Avoid the usage of Si, prefer Sim
Details on Acronym: Si
Si (Simeis obs.)
***** Avoid the usage of Si, prefer Sim
Details on Acronym: Sim
Sim (Simeis obs.)= (S) = (SG) = (Sh) = (Shajn) = (SHZ) = (Si) = (Simeis) = (Simeiz)
Write:<<Sim NNN>>
<<Sim 306>>
N: 306
Object:HII (SIMBAD class: HIIReg = HII Region)
Note:Sim 22 is a PN = PN G128.0-04.1 = PK 128-04 1.
Sim 31 is not real (Gaze + Shajn, 1954)
Sim 106, 302, 303, 304 are defined nowhere.
Sim 147 is a wellknown galactic SNR, often found as 'S 147'.
The synonym 'S' is of current use for 'Sh 2-' except in eastern Europa where it generally stands for Sim.
Ref:=1950IzKry...6....3S
bySHAJN G.A.
, GAZE V.F.
Izv. Krym. Astrofiz. Obs., 6, 3-27 (1950)
A few results of the study of emissive galactic nebulae.
oNumbering 'NN' in Table 1, col(1) is not used in SIMBAD
oTable 1, col(2): <Sim NN> (Nos 1-19)
Ref:=1951IzKry...7...93G
byGAZE V.F.
, SHAJN G.A.
Izv. Krym. Astrofiz. Obs., 7, 93-98 (1951)
Second list of diffuse nebulae.
oNumbering 'NN' in Table, col(1) is not used in SIMBAD
oTable, col(2): <Sim NNN> (Nos 20-105)
Ref:=1952IzKry...8...17G
byGAZE V.F.
, SHAJN G.A.
Izv. Krym. Astrofiz. Obs., 8, 17-18 (1952)
Two new filamentary nebulae near omi 02 and omi 01 Cyg.
oText: <Sim NNN> (Nos 107-108)
Ref:=1952IzKry...9...52G
byGAZE V.F.
, SHAJN G.A.
Izv. Krym. Astrofiz. Obs., 9, 52-67 (1952)
Third list of diffuse emission nebulae.
oNumbering 'NNN' in Table, col(1) is not used in SIMBAD
oTable, col(2): <Sim NNN> (Nos 109-279)
Ref:=1954IzKry..11...39G
byGAZE V.F.
, SHAJN G.A.
Izv. Krym. Astrofiz. Obs., 11, 39-41 (1954)
Fourth list of diffuse emission nebulae.
oNumbering 'NN' in Table, col(1) is not used in SIMBAD
oTable, col(2): <Sim NNN> (Nos 280-301)
Details on Acronym: Sim
Sim (Simeis obs.)= (S) = (Si) = (Simeis) = (Simeiz)
Write:<<Sim HHMM+DD.N>>
N: 121
Object:(Rad) (SIMBAD class: Radio = Radio Source)
Ref:=1971ATsir.665....1L
byLARIONOV M.G.
, GORSHKOV A.G., POPOV M.V., MOISEEV I.G.
Astron. Tsirk., 665, 1-6 (1971)
The fast survey of the sky at frequency 8550 MHz in the range of
declination +0 to +30.
oSIM
oTable: <Sim HHMM+DD.N> N=121
Details on Acronym: Simeis
Simeis (Simeis obs.)
***** Avoid the usage of Simeis, prefer Sim
Details on Acronym: Simeis
Simeis (Simeis obs.)
***** Avoid the usage of Simeis, prefer Sim
Details on Acronym: Simeiz
Simeiz (Simeis obs.)
***** Avoid the usage of Simeiz, prefer Sim
Details on Acronym: Simeiz
Simeiz (Simeis obs.)
***** Avoid the usage of Simeiz, prefer Sim
Details on Acronym: Cl* NGC 5904 Sim
Cl* NGC 5904 Sim (Simoda)
Write:<<Cl* NGC 5904 Sim NNN>>
Object:*inCl
Rem:Stars from a private comm. of Simoda M., 1981.
Ref:=1993AJ....105..173S
bySMITH G.H.
, NORRIS J.E.
Astron. J., 105, 173-183 (1993)
CN variations among asymptotic giant branch and horizontal branch
stars in the intermediate metallicity globular clusters M5, M4, and NGC 6752.
oTable 1: Stars 'SNNN' (Cl* NGC 5904 SIM NNN in SIMBAD) are from a private comm. of Simoda M., 1981.
oTable 1: <Cl* NGC 5904 SIM NNN> N=2 (Nos 344, 445).