Details on Acronym: MMS | |
| MMS | (mm Source) |
| ***** | Avoid the usage of MMS, prefer [WZM2000] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [WZM2000] | |
| [WZM2000] | (Ward-Thompson+Zylka+Mezger+, 2000)= (MMS) |
| Write: | <<[WZM2000] MMS NA>> |
| N: | 5+4+3 |
| Object: | (mm) (SIMBAD class: mmRad = Millimetric Radio Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | Observations of a ridge of bright submillimeter and millimeter emission n NGC 2264, designated 'NAME NGC 2264 MM. Within the ridge authors discover a cluster of 5 smm sources. In SMM 4 and 5, different clumps 'MMS NA' are found in 2003ApJ...599..335S. |
| in source: | NGC 2264 |
| Ref: | =2000A&A...355.1122W |
| by | WARD-THOMPSON D. , ZYLKA R., MEZGER P.G., SIEVERS A.W. |
| Astron. Astrophys., 355, 1122-1128 (2000) | |
| Dust emission from star-forming regions. VI. The submillimetre YSO cluster in NGC 2264. | |
| o | <NAME NGC 2264 MM>. Table 2: <[WZM2000] MMS N> (Nos 1-5). |
| Ref: | =2003ApJ...599..335S |
| by | SCHREYER K. , STECKLUM B., LINZ H., HENNING T. |
| Astrophys. J., 599, 335-341 (2003) | |
| NGC 2264 IRS 1: the central engine and its cavity. | |
| o | Fig.1: [SSL2003] Object 1 to 7 = [TCY98] 1 to 7. |
| o | Fig.1: <[SSL2003] Object NN> (Nos 1-13), <[TCY98] N> (No. 7 added). Fig.5b, Table 1: <[SSL2003] AN> (Nos S1-S3, C1). Fig.5c: <[SSL2003] Outflow Na> (Nos 1, 2a-2b, 3), <[SSL2003] Blue Blob> N=1. Fig.5a: <[WZM2000] MMS NA> (Nos 4A-4D, 5A-5C) added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |