The interstellar medium local to HD 10125 (O9.7II)
2003 ◽
Vol 212
◽
pp. 700-701
Keyword(s):
The structure and dynamics of the interstellar medium (ISM) are strongly affected by the action of massive stars. They deposit in the ISM a huge number of ionizing photons and transfer to it vast amounts of mechanical energy via their powerful stellar winds. As a consequence, massive stars create what is known as an interstellar bubble, i.e., a minimum in the gas distribution characterized by a low volume density and a high temperature, surrounded by an expanding envelope (Weaver et al. 1977). The star should be seen projected onto, or close to, the centre of the H i minimum.
1984 ◽
Vol 105
◽
pp. 299-319
Keyword(s):
2008 ◽
Vol 4
(S252)
◽
pp. 317-327
◽
Keyword(s):
1999 ◽
Vol 16
(1)
◽
pp. 106-112
◽
Keyword(s):
Keyword(s):