TY - JOUR
T1 - The G305 Star-forming Region. I. Newly Classified Hot Stars
AU - Borissova, Jura
AU - Roman-Lopes, Alexandre
AU - Covey, Kevin R.
AU - Medina, Nicolas
AU - Kurtev, Radostin
AU - Roman-Zuniga, Carlos
AU - Kuhn, M. A.
AU - Contreras Peña, Carlos
AU - Lucas, Philip
AU - Ramirez Alegria, Sebastian
AU - Minniti, Dante
AU - Kounkel, Marina
AU - Stringfellow, Guy
AU - Barbá, Rodolfo H.
AU - Suárez, Genaro
PY - 2019/7/1
Y1 - 2019/7/1
N2 - The relatively nearby star-forming complex G305 is one of the most luminous H II regions in the Galaxy, and it contains several sites and epochs of star formation. Using a combination of near-infrared photometry from “Vista Variables in Via Lactea” ESO Large Public Survey, SDSS-IV APOGEE-2 spectra, and Gaia DR2 photometry and astrometry, we report on 29 OB type, Wolf-Rayet, and emission-line stars, 18 of which are newly classified. Most of these hot stars belongs to the main sequence, although some stars of class I are also proposed. The mean radial velocity is RV = -41.8 {km} {{{s}}}-1. The average spectroscopic distance is 3.2 ± 1.6 kpc, while the Gaia DR2 average distance is 3.7 ± 1.8 kpc. Eight objects show light-curve variations with amplitudes greater than 0.5 mag in the K S band. Based on Vista Variables in the Vía Láctea (VVV); SDSS-IV APOGEE-2 and Gaia DR2 data.
AB - The relatively nearby star-forming complex G305 is one of the most luminous H II regions in the Galaxy, and it contains several sites and epochs of star formation. Using a combination of near-infrared photometry from “Vista Variables in Via Lactea” ESO Large Public Survey, SDSS-IV APOGEE-2 spectra, and Gaia DR2 photometry and astrometry, we report on 29 OB type, Wolf-Rayet, and emission-line stars, 18 of which are newly classified. Most of these hot stars belongs to the main sequence, although some stars of class I are also proposed. The mean radial velocity is RV = -41.8 {km} {{{s}}}-1. The average spectroscopic distance is 3.2 ± 1.6 kpc, while the Gaia DR2 average distance is 3.7 ± 1.8 kpc. Eight objects show light-curve variations with amplitudes greater than 0.5 mag in the K S band. Based on Vista Variables in the Vía Láctea (VVV); SDSS-IV APOGEE-2 and Gaia DR2 data.
KW - Galaxy: stellar content
KW - infrared: stars
KW - stars: massive
KW - stars: Wolf–Rayet
KW - stars: variables: general
U2 - 10.3847/1538-3881/ab276b
DO - 10.3847/1538-3881/ab276b
M3 - Article
SN - 0004-6256
VL - 158
JO - The Astronomical Journal
JF - The Astronomical Journal
M1 - 46
ER -