Details on Acronym: MM | |
MM | (Millimeter source) |
***** | Avoid the usage of MM, prefer [S2001] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [S2001] | |
[S2001] | (Shepherd, 2001)= (MM) = [S2001a] |
Write: | <<[S2001] MM N>> |
N: | 9 |
Object: | (mm) (SIMBAD class: mmRad = Millimetric Radio Source) |
Stat: | is completely incorporated in Simbad |
in source: | W 75:W 75N = W 75N |
Ref: | =2001ApJ...546..345S |
by | SHEPHERD D.S. |
Astrophys. J., 546, 345-351 (2001) | |
Warm dust emission near W75 N IRS1: evidence for multiple energetic outflows. | |
o | W75 N IRS1 = [YST88] IRS 1 |
o | Table 2, Fig.1: <[S2001] MM N> (Nos 1-4). |
Ref: | =2003ApJ...584..882S |
by | SHEPHERD D.S. , TESTI L., STARK D.P. |
Astrophys. J., 584, 882-894 (2003) | |
Clustered star formation in W75 N. | |
o | Fig.2: <[STS2003] WW-A> (Nos SW-A to SW-K, C-A to C-B, NE-A to NE-I). Fig.5, Table 1: <[S2001] MM N> (Nos 5-9) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [S2001a] | |
[S2001a] | (Shepherd, 2001) |
***** | Avoid the usage of [S2001a], prefer [S2001] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |