Stellar formation in HI interstellar bubbles around massive stars
2006 ◽
Vol 2
(S237)
◽
pp. 444-444
Keyword(s):
Stellar winds from O and WR stars transfer large amounts of mechanical energy and momentum into the interstellar medium. They sweep up and compress the interstellar material, creating interstellar bubbles. These structures are detected as optical ring nebulae, as thermal radio continuum sources, as infrared shells, as neutral gas voids and expanding shells in the HI line emission distribution, and as molecular shells.
1993 ◽
Vol 155
◽
pp. 347-347
Keyword(s):
2007 ◽
Vol 3
(S242)
◽
pp. 180-181
Keyword(s):
2005 ◽
Vol 436
(1)
◽
pp. 155-163
◽
1999 ◽
Vol 51
(6)
◽
pp. 751-764
◽
Keyword(s):
2008 ◽
pp. 322-325
◽
2003 ◽
Vol 212
◽
pp. 732-733
Keyword(s):
1996 ◽
Vol 169
◽
pp. 619-620
Keyword(s):
2020 ◽
Vol 499
(2)
◽
pp. 1788-1794
Keyword(s):
Keyword(s):