Details on Acronym: FIR | |
FIR | (Far IR) |
***** | Avoid the usage of FIR, prefer [MCK88] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [MCK88] | |
[MCK88] | (Mezger+Chini+Kreysa+, 1988)= (FIR) |
Write: | <<[MCK88] NGC 2024 FIR N>> <<[MCK88] NGC 2024 Ext WW>> <<[MCK88] S255IR FIR NA>> |
N: | 7+2+5 |
Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
Stat: | is completely incorporated in Simbad |
Note: | 'NGC 2024 FIR N', (Nos 1-7), FIR in NGC 2024. 'NGC 2024 Ext WW', (Nos NS, EW), N=2 sources ext. to NGC 2024. See also [WGW97] and lcgr. 'S255IR FIR NA', (Nos 1C, 1E, 2C, 2E, 3), C for Core and E for envelope, N=5 sources in Sh 2-255. |
in source: | NGC 2024 |
in source: | SH 2-255 |
Ref: | =1988A&A...191...44M |
by | MEZGER P.G. , CHINI R., KREYSA E., WINK J.E., SALTER C.J. |
Astron. Astrophys., 191, 44-56 (1988) | |
Dust emission at submillimeter wavelengths from cloud cores and protostellar condensations in NGC 2024 and S 255IR. | |
o | Table 2: <[MCK88] NGC 2024 FIR N> N=6, <[MCK88] NGC 2024 Ext WW> N=2, <[MCK88] S255IR FIR NA> N=5 |
Ref: | =1992A&A...256..631M |
by | MEZGER P.G. , SIEVERS A.W., HASLAM C.G.T., KREYSA E., LEMKE R., MAUERSBERGER R., WILSON T.L. |
Astron. Astrophys., 256, 631-639 (1992) | |
Dust emission from star forming regions. II. The NGC 2024 cloud - core revisited. | |
o | <[MCK88] NGC 2024 FIR 7> |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |