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 |
by | BEICHMAN C.A. , BECKLIN E.E., WYNN-WILLIAMS C.G. |
Astrophys. J., 232, 47-51 (1979) | |
New multiple systems in molecular clouds. | |
o | Table 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 |
by | SIMON 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. | |
o | in ref list Simon et al 1981a is wrong |
o | Table 2: <[SFC83] S140 N> (Nos 4-5) = <[BBW79] S140 IRS N> (Nos 4-5). |
Ref: | =1989ApJ...338L..25S |
by | SCHWARTZ P.R. |
Astrophys. J., 338, 25-28 (1989) | |
Jets and bullets in S 140. | |
o | Table 1: <[BBW79] S 140 IRS NW> (Nos 2N and 2S) added. |
Ref: | =1998ApJ...500..320Y |
by | YAO 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. | |
o | VLA 4 = [BBW79] S 140 IRS 4 = [SFC83] S140 4. |
o | Fig.1: <[BBW79] S 140 WW> (No. SE). |
Ref: | =2001ApJ...561..282K |
by | KRAEMER 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. | |
o | Table 4: <KJD NN> (Nos 1-11). Text: <[BBW79] S140 IRS N> (Nos 6-7) added. |
Ref: | =2001A&A...378..539P |
by | PREIBISCH 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. | |
o | Fig.1: <[BBW79] S 140 IRS 3a> (Nos 3a to 3c). Fig.1: <[PBS2001] A> (Nos A-F). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: IRS | |
IRS | (IR Source) |
***** | Avoid the usage of IRS, prefer [BBW79] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: IRS | |
IRS | (IR Source) |
***** | Avoid the usage of IRS, prefer [BBW79] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: R | |
R | (Radio) |
***** | Avoid the usage of R, prefer [BBW79] |
Origin | of the Acronym: A = Assigned by the author(s) |