Massive star-formation toward G28.87+0.07
2012 ◽
Vol 8
(S287)
◽
pp. 180-181
Keyword(s):
AbstractWe investigated the high-mass star-forming region G28.87+0.07 by means of maser kinematics, including H2O, CH3OH, and OH, and radio to infrared, continuum observations. All observational evidence suggests that these masers are associated with the same young star of 20-30 M⊙, still in the main accretion phase and surrounded by a rich stellar cluster.
Keyword(s):
2012 ◽
Vol 8
(S287)
◽
pp. 184-185
Keyword(s):
2002 ◽
Vol 206
◽
pp. 147-150
Keyword(s):
2017 ◽
Vol 13
(S336)
◽
pp. 323-324
Keyword(s):
Keyword(s):
2019 ◽
Vol 492
(1)
◽
pp. 1335-1347
Keyword(s):