Details on Acronym: [CLM2017] | |
[CLM2017] | (Contreras Pena+Lucas+Minniti+, 2017)= (VVVv) |
Write: | <<[CLM2017] VVVvNNN>> |
Object: | V* (SIMBAD class: Variable* = Variable Star) |
Note: | N=816 high-amplitude infrared variable stars (ΔKs>1mg) in the VISTA Variables in the Via Lactea (VVV) survey. |
Ref: | =2017MNRAS.465.3011C |
by | CONTRERAS PENA C. , LUCAS P.W., MINNITI D., KURTEV R., STIMSON W., NAVARRO MOLINA C., BORISSOVA J., KUMAR M.S.N., THOMPSON M.A., GLEDHILL T., TERZI R., FROEBRICH D., CARATTI O GARATTI A. |
Mon. Not. R. Astron. Soc., 465, 3011-3038 (2017) | |
A population of eruptive variable protostars in VVV. | |
o | Table 2, col(1): <[CLM2017] VVVvNNN> (Nos VVVv1-VVVv816). |
=E= | Catalogue in electronic form as <J/MNRAS/465/3011/> |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: VVVv | |
VVVv | (VISTA Variables in the Via Lactea variable) |
***** | Avoid the usage of VVVv, prefer [CLM2017] |
Origin | of the Acronym: A = Assigned by the author(s) |