Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati BBW79] S 255 IRS$
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Details on Acronym:   [BBW79]
  
[BBW79] (Beichman+Becklin+Wynn-Williams, 1979)= (IRS) = (R)
Write:<<[BBW79] Cep A N>>
<<[BBW79] S 140 IRS Na>>
<<[BBW79] S 140 IRS NW>>
<<[BBW79] S 140 WW>>
<<[BBW79] S 140 N>>
<<[BBW79] S 255 IRS N>>
N: 16
Object:(Rad) + (IR)  (SIMBAD class: Infrared = Infra-Red Source)
Stat:is completely incorporated in Simbad
Note:N=3 radio-sources in Cep A MCld, format 'Cep A N', (Nos 1-3) sometimes found in the literature with a format 'R1 to R3'
N=7 (IR) sources in Sh 2-140, format 'S 140 IRS N', (Nos 1-7), No. 3 is resolved in 3 point sources 3a to 3c, Nos 4 and 5 are also designated as [SFC83] VLA sources. and different (Nos 4-7) are created in 2002A&A...381..905W, designated as [WBP2002] in SIMBAD.
N=2 radio-source in Sh 2-140, format 'S 140 WW' also designated as 'VLA NW' and 'VLA SE'.
N=2 (IR) sources in Sh 2-255, format 'S 255 IRS N', (Nos 1-2), same as [HPF97] IRS 1 and 2.
in source:NAME Cep A
in source:SH 2-140
in source:SH 2-255
Ref:=1979ApJ...232L..47B
byBEICHMAN C.A. , BECKLIN E.E., WYNN-WILLIAMS C.G.
 Astrophys. J., 232, 47-51 (1979)
  New multiple systems in molecular clouds.
oTable 1: <[BBW79] Cep A N> (Nos 1-3), <[BBW79] S 140 IRS N> (Nos 1-3), <[BBW79] S 140 WW> (No. NW), <[BBW79] S 255 IRS N> (Nos 1-2).
Ref:=1983ApJ...266..623S
bySIMON M. , FELLI M., CASSAR L., FISCHER J., MASSI M.
 Astrophys. J., 266, 623-645 (1983)
  Infrared line and radio continuum emission of circumstellar ionized regions.
oin ref list Simon et al 1981a is wrong
oTable 2: <[SFC83] S140 N> (Nos 4-5) = <[BBW79] S140 IRS N> (Nos 4-5).
Ref:=1989ApJ...338L..25S
bySCHWARTZ P.R.
 Astrophys. J., 338, 25-28 (1989)
  Jets and bullets in S 140.
oTable 1: <[BBW79] S 140 IRS NW> (Nos 2N and 2S) added.
Ref:=1998ApJ...500..320Y
byYAO Y. , ISHII M., NAGATA T., OGAWA Y., SATO S., WATANABE M., YAMASHITA T.
 Astrophys. J., 500, 320-328 (1998)
  Near-infrared polarimetric study of S140 IRS.
oVLA 4 = [BBW79] S 140 IRS 4 = [SFC83] S140 4.
oFig.1: <[BBW79] S 140 WW> (No. SE).
Ref:=2001ApJ...561..282K
byKRAEMER K.E. , JACKSON J.M., DEUTSCH L.K., KASSIS M., HORA J.L., FAZIO G.G., HOFFMANN W.F., DAYAL A.
 Astrophys. J., 561, 282-298 (2001)
  Dust characteristics of massive star-forming sites in the mid-infrared.
oTable 4: <KJD NN> (Nos 1-11). Text: <[BBW79] S140 IRS N> (Nos 6-7) added.
Ref:=2001A&A...378..539P
byPREIBISCH T. , BALEGA Y.Y., SCHERTL D., SMITH M.D., WEIGELT G.
 Astron. Astrophys., 378, 539-545 (2001)
  High-resolution near-infrared study of the deeply embedded young stellar object S140 IRS3.
oFig.1: <[BBW79] S 140 IRS 3a> (Nos 3a to 3c). Fig.1: <[PBS2001] A> (Nos A-F).
Originof the Acronym: S = Created by Simbad, the CDS Database

Details on Acronym:   IRS
  
IRS (IR Source)
***** Avoid the usage of IRS, prefer [BBW79]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   IRS
  
IRS (IR Source)
***** Avoid the usage of IRS, prefer [BBW79]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   R
  
R (Radio)
***** Avoid the usage of R, prefer [BBW79]
Originof the Acronym: A = Assigned by the author(s)