Details on Acronym: MIR | |
MIR | (Mid-IR) |
***** | Avoid the usage of MIR, prefer [SSG2002] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: MMS | |
MMS | (mm Source) |
***** | Avoid the usage of MMS, prefer [SSG2002] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [SSG2002] | |
[SSG2002] | (Stanke+Smith+Gredel+, 2002)= (MIR) = (MMS) |
Write: | <<[SSG2002] MMS NA>> <<[SSG2002] MIR N>> |
N: | 1+4+5 |
Object: | (mm) + (Mid IR) (SIMBAD class: mmRad = Millimetric Radio Source) |
Stat: | is completely incorporated in Simbad |
Note: | Discovey of a new millimeter sources with 4 sub-components, and of 4 Mid-IR sources in LDN 1616. |
in source: | LDN 1616 |
Ref: | =2002A&A...393..251S |
by | STANKE T. , SMITH M.D., GREDEL R., SZOKOLY G. |
Astron. Astrophys., 393, 251-258 (2002) | |
Triggered star formation in Orion cometary clouds? I. The case of L1616. | |
o | Fig.3, Table 1: <[SSG2002] MMS N> (No. 1), <[SSG2002] MMS 1A> (Nos 1A-1D). Fig.4, Table 1: <[SSG2002] MIR N> (Nos 1-5). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |