Details on Acronym: [CBW2017] | |
| [CBW2017] | (Csengeri+Bontemps+Wyrowski+, 2017) |
| Write: | <<[CBW2017] GLLL.llll+BB.bbbb-MMN>> <<[CBW2017] LLL.llll+B.bbbb-MMN>> (not recognised by Simbad, but found in literature) |
| N: | 100 |
| Object: | Clump (SIMBAD class: smmRad = Sub-Millimetric Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | ALMA Band 7 Cycle 2 observations of N=100 sources in 35 infrared-quiet massive clumps selected from the ATLASGAL survey. |
| Ref: | =2017A&A...600L..10C |
| by | CSENGERI T. , BONTEMPS S., WYROWSKI F., MOTTE F., MENTEN K.M., BEUTHER H., BRONFMAN L., COMMERCON B., CHAPILLON E., DUARTE-CABRAL A., FULLER G.A., HENNING T., LEURINI S., LONGMORE S., PALAU A., PERETTO N., SCHULLER F., TAN J.C., TESTI L., TRAFICANTE A., URQUHART J.S. |
| Astron. Astrophys., 600L, 10-10 (2017) | |
| ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumps. | |
| o | Fig. A.1, Table A.1: <[CBW2017] GLLL.llll+BB.bbbb-MMN> N=100. |
| =E= | Catalogue in electronic form as <J/A+A/600/L10/> |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |