Details on Acronym: [KHM2017] | |
[KHM2017] | (Kounkel+Hartmann+Mateo+, 2017) |
Write: | <<[KHM2017] {NGC20}{6|2}{3|4|8} {RV}NNNNa>> <<[KHM2017] L1622 RVNNNN>> |
N: | 292 |
Object: | * (SIMBAD class: Star) |
Note: | Magellan Clay telescope M2FS spectroscopy of N=292 stars in the fields of N=4 cluster in the Orion B molecular cloud. See also [KHT2016]. |
in source: | NGC 2023 |
in source: | NGC 2024 |
in source: | NGC 2068 |
in source: | LDN 1622 |
Ref: | =2017ApJ...844..138K |
by | KOUNKEL M. , HARTMANN L., MATEO M., BAILEY III J.I. |
Astrophys. J., 844, 138-138 (2017) | |
Kinematics of the optically visible YSOs toward the Orion B molecular cloud. | |
o | Table 2: <[KHM2017] NGC2023 RVNNNN> N=107 among (Nos 2533-2649), <[KHM2017] NGC2024 RVNNNNa> N=48 among (Nos 2622-2686, 2670a, 2670b), <[KHM2017] NGC2068 RVNNNNa> (Nos 2687-2766, 2734a, 2734b), <[KHM2017] L1622 RVNNNN> (Nos 2767-2825). |
=E= | Catalogue in electronic form as J/ApJ/844/138 |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |