Details on Acronym: [TLO2017] | |
[TLO2017] | (Tatematsu+Liu+Ohashi+, 2017) |
Write: | <<[TLO2017] GLLL>> <<[TLO2017] GLLLWW>> <<[TLO2017] GLLLWN>> <<[TLO2017] GLLL.lW>> <<[TLO2017] G202.0M>> |
N: | 2+13+16+3+1+1 |
Object: | Dense Core (SIMBAD class: denseCore = Dense Core) |
Stat: | is completely incorporated in Simbad |
Note: | JCMT SCUBA-2 and Nobeyama 45m telescope observations of N=35 dense cores toward Planck cold clumps. |
Ref: | =2017ApJS..228...12T |
by | TATEMATSU K. , LIU T., OHASHI S., SANHUEZA P., NGUYEN LU'O'NG Q., HIROTA T., LIU S.-Y., HIRANO N., CHOI M., KANG M., THOMPSON M.A., FULLER G., WU Y., LI D., DI FRANCESCO J., KIM K.-T., WANG K., RISTORCELLI I., JUVELA M., SHINNAGA H., CUNNINGHAM M., SAITO M., LEE J.-E., TOTH L.V., HE J., SAKAI T., KIM J., (The JCMT Large Program "SCOPE" Collaboration), (The TRAO Key Science Program "TOP" Collaboration) |
Astrophys. J., Suppl. Ser., 228, 12-12 (2017) | |
Astrochemical properties of Planck cold clumps. | |
o | Figs 1-14, Table 3: <[TLO2017] GLLL> N=2, <[TLO2017] GLLLWW> N=13, <[TLO2017] GLLLWN> N=16, <[TLO2017] GLLL.lW> N=3, <[TLO2017] G202.0M> N=1. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |