Details on Acronym: [VNT2022] | |
| [VNT2022] | (van Gelder+Nazari+Tabone+, 2023) |
| Write: | <<[VNT2022] NNNNNNA>> <<[VNT2022] GLLL.llll+BB.bbbbAN>> |
| N: | 68+14 |
| Object: | Protostar (SIMBAD class: YSO = Young Stellar Object) |
| Note: | ALMA band 6 continuum and CH3OH line observations of N=68+14 protostars in high-mass protostellar cores. Use of archival ALMA Evolutionary study of High Mass Protocluster Formation in the Galaxy survey (ALMAGAL) data. |
| Ref: | =2022A&A...662A..67V |
| by | VAN GELDER M.L. , NAZARI P., TABONE B., AHMADI A., VAN DISHOECK E.F., BELTRAN M.T., FULLER G.A., SAKAI N., SANCHEZ-MONGE A., SCHILKE P., YANG Y.-L., ZHANG Y. |
| Astron. Astrophys., 662A, 67-67 (2022) | |
| Importance of source structure on complex organics emission. I. Observations of CH_{3}OH from low-mass to high-mass protostars. | |
| o | Tables A.1-A.2: <[VNT2022] NNNNNNA> N=68, <[VNT2022] GLLL.llll+BB.bbbbAN> N=14. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |