Massive Star Formation Throughout the Galactic Disk
2009 ◽
Vol 5
(H15)
◽
pp. 798-798
Keyword(s):
AbstractHigh-mass star formation is manifestly a phenomenon of the Galactic Plane. The process begins with pre-stellar cores, evolves to proto-stellar objects, and culminates in massive main-sequence stars. Because massive young stellar objects are deeply embedded, the radio, sub-mm, and far/mid-infrared spectral windows are the most revealing. Galactic plane surveys at these wavelengths trace hot and cold molecular gas, interstellar masers, warm dust, and ionized gas that are present during star formation.
2019 ◽
Vol 71
(2)
◽
Keyword(s):
2007 ◽
Vol 3
(S242)
◽
pp. 130-134
◽
2020 ◽
Vol 500
(4)
◽
pp. 4448-4468
Keyword(s):
Keyword(s):
Keyword(s):
2012 ◽
Vol 8
(S292)
◽
pp. 50-50
Keyword(s):
2018 ◽
Vol 56
(1)
◽
pp. 41-82
◽
Keyword(s):