Induced Star Formation in M17: High Resolution NH3 and IR Observations
1987 ◽
Vol 115
◽
pp. 141-142
Keyword(s):
The West
◽
A VLA radio continuum study of the H II region M17 (Felli, Churchwell and Massi, 1984) has shown the presence of an elongated sharp arc structure in the South Bar of the nebula, in a region of heavy obscuration. The arc has been interpreted as an ionization boundary, viewed edge on, located between the diffuse H II region, to the east, and a dense component of the extended molecular cloud, to the west. About 3″ to the west of this arc, an ultra-compact H II region has been found. This has a shell type structure, a linear diameter of 0.004 pc and probably is the result of induced star formation in the molecular cloud produced by the pressure front preceding the ionization front.
2016 ◽
Vol 11
(S322)
◽
pp. 133-136
Keyword(s):
2013 ◽
Vol 9
(S303)
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pp. 464-466
Keyword(s):
1991 ◽
Vol 147
◽
pp. 229-233
Keyword(s):
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Keyword(s):
1985 ◽
Vol 106
◽
pp. 551-558
Keyword(s):
1989 ◽
Vol 120
◽
pp. 128-128
Keyword(s):
1987 ◽
Vol 115
◽
pp. 143-145
Keyword(s):