Details on Acronym: [FLC2020] | |
| [FLC2020] | (Feng+Li+Caselli+, 2020) |
| Write: | <<[FLC2020] GLLL.ll+BB.bb PN>> <<[FLC2020] GLL.ll+B.bb PN>> (not recognised by Simbad, but found in literature) |
| N: | 12 |
| Object: | Core (SIMBAD class: denseCore = Dense Core) |
| Stat: | is completely incorporated in Simbad |
| Note: | IRAM 30 m and NRO 45 m telescopes observations of N=12 peaks in the field of four regions, as part of the Multiwavelength line-Imaging survey of the 70µm-dArk and bright clOuds (MIAO). |
| Ref: | =2020ApJ...901..145F |
| by | FENG S. , LI D., CASELLI P., DU F., LIN Y., SIPILA O., BEUTHER H., SANHUEZA P., TATEMATSU K., LIU S.Y., ZHANG Q., WANG Y., HOGGE T., JIMENEZ-SERRA I., LU X., LIU T., WANG K., ZHANG Z.Y., ZAHORECZ S., LI G., LIU H.B., YUAN J. |
| Astrophys. J., 901, 145-145 (2020) | |
| The chemical structure of young high-mass star-forming clumps. II. Parsec-scale CO depletion and deuterium fraction of HCO^+. | |
| o | Fig. 1, Table 2: <[FLC2020] GLLL.ll+BB.bb PN> N=12. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |