Details on Acronym: [MBA2020] | |
| [MBA2020] | (Mottram+Beuther+Ahmadi+, 2020) |
| Write: | <<[MBA2020] Cold Core N>> |
| N: | 2 |
| Object: | Core (SIMBAD class: denseCore = Dense Core) |
| Stat: | is completely incorporated in Simbad |
| Note: | NOEMA 1.4mm and IRAM 30m telescope EMIR observations of N=2 cold cores in [WBN72] W 3 IRS 4. |
| in source: | W 3:[WBN72] W 3 IRS 4 = [WBN72] W 3 IRS 4 |
| Ref: | =2020A&A...636A.118M |
| by | MOTTRAM J.C. , BEUTHER H., AHMADI A., KLAASSEN P.D., BELTRAN M.T., CSENGERI T., FENG S., GIESER C., HENNING T., JOHNSTON K.G., KUIPER R., LEURINI S., LINZ H., LONGMORE S.N., LUMSDEN S., MAUD L.T., MOSCADELLI L., PALAU A., PETERS T., PUDRITZ R.E., RAGAN S.E., SANCHEZ-MONGE A., SEMENOV D., URQUHART J.S., WINTERS J.M., ZINNECKER H. |
| Astron. Astrophys., 636A, 118-118 (2020) | |
| From clump to disc scales in W3 IRS4. A case study of the IRAM NOEMA large programme CORE. | |
| o | Fig. 2, Table 2: <[MBA2020] Cold Core N> (Nos 1-2). |
| Origin | of the Acronym: D = Assigned by the Dictionary of Acronyms |