Details on Acronym: [KKY2019] | |
| [KKY2019] | (Koyama+Koyama+Yamashita+, 2019) |
| Write: | <<[KKY2019] {d|e}NN>> |
| N: | 13+15 |
| Object: | G (SIMBAD class: Galaxy) |
| Stat: | is completely incorporated in Simbad |
| Note: | Nobeyama 45m radio telescope CO(1-0) observations of N=13+15 green valley galaxies. |
| Ref: | =2019ApJ...874..142K |
| by | KOYAMA S. , KOYAMA Y., YAMASHITA T., HAYASHI M., MATSUHARA H., NAKAGAWA T., NAMIKI S.V., SUZUKI T.L., FUKAGAWA N., KODAMA T., LIN L., MOROKUMA-MATSUI K., SHIMAKAWA R., TANAKA I. |
| Astrophys. J., 874, 142-142 (2019) | |
| Do galaxy morphologies really affect the efficiency of star formation during the phase of galaxy transition? | |
| o | Table 1: <[KKY2019] dNN> (Nos d1-13), <[KKY2019] eNN> (Nos e1-e15). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |