Details on Acronym: FIR | |
FIR | (Far IR) |
***** | Avoid the usage of FIR, prefer [MWZ90] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [MWZ90] | |
[MWZ90] | (Mezger+Wink+Zylka, 1990)= (FIR) |
Write: | <<[MWZ90] OMC-1 FIR N>> <<[MWZ90] OMC-2 FIR Na>> |
N: | 4+6+18 |
Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
Stat: | is completely incorporated in Simbad |
Note: | N=4 Far-IR sources in OMC 1, format 'OMC-1 FIR N'. N=6 Far-IR sources in OMC 2, format 'OMC-2 FIR N' and N=18 components format 'OMC-2 FIR Na'. |
in source: | OMC:OMC 1 = OMC 1 |
in source: | OMC:OMC 2 = OMC 2 |
Ref: | =1990A&A...228...95M |
by | MEZGER P.G. , WINK J.E., ZYLKA R. |
Astron. Astrophys., 228, 95-107 (1990) | |
Lambda 1.3 mm dust emission from the star-forming cloud cores OMC 1 and 2. | |
o | Table 1: <[MWZ90] OMC-1 FIR N> N=4, <[MWZ90] OMC-2 FIR N> N=6 |
Ref: | =1997ApJ...474L.135C |
by | CHINI R. , REIPURTH B., WARD-THOMPSON D., BALLY J., NYMAN L.-A., SIEVERS A., BILLAWALA Y. |
Astrophys. J., 474, 135-138 (1997) | |
Dust filaments and star formation in OMC-2 and OMC-3. | |
o | Table 1: <[CRW97] OMC-3 MMS NN> (Nos 1-10). Table 1: <[MWZ90] OMC-2 FIR Na> (Nos 1a-1c, 6a-6d) |
Ref: | =2008ApJ...683..255S |
by | SHIMAJIRI Y. , TAKAHASHI S., TAKAKUWA S., SAITO M., KAWABE R. |
Astrophys. J., 683, 255-266 (2008) | |
Millimeter- and submillimeter-wave observations of the OMC-2/3 region. II. Observational evidence for outflow-triggered star formation in the OMC-2 FIR 3/4 region. | |
o | Fig.7, Table 4: <[MWZ90] OMC-2 FIR 4a> (Nos 4a-4k) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |