1D, 2D and 3D Collapse of Interstellar Clouds
1980 ◽
Vol 58
◽
pp. 235-246
Keyword(s):
B Stars
◽
This review is concerned with recent theoretical investigations and numerical models of star formation with varions symmetries. Observations strongly support the fact that stars condense out of cool (≈10 K) and dense (103-104 atoms/cm3) interstellar clouds due to gravitational instability and collapse. Bright, young stellar objects (0- and B-stars are always found in the vicinity of coloud complexes.
2006 ◽
Vol 2
(S237)
◽
pp. 192-198
2020 ◽
Vol 500
(4)
◽
pp. 4448-4468
Keyword(s):
2020 ◽
Vol 496
(1)
◽
pp. 870-874
Keyword(s):
Keyword(s):
2019 ◽
Vol 487
(2)
◽
pp. 1517-1528
◽
Keyword(s):
2019 ◽
Vol 489
(1)
◽
pp. 52-77
Keyword(s):
1999 ◽
Vol 51
(6)
◽
pp. 791-818
◽
2006 ◽
Vol 2
(S237)
◽
pp. 217-221
Keyword(s):
2021 ◽
Vol 507
(4)
◽
pp. 5106-5131