Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265..778b&link_type=abstract
Astrophysical Journal, Part 1, vol. 265, Feb. 15, 1983, p. 778-790.
Astronomy and Astrophysics
Astronomy
85
Hydrogen Clouds, Interstellar Gas, Ionized Gases, Molecular Clouds, Nebulae, Astronomical Maps, Infrared Astronomy, Interferometry, Orion Nebula, Radio Sources (Astronomy), Stellar Winds
Scientific paper
The star-forming regions NGC 2071, CRL 961, S106 IR, and S87, contain compact continuum radio sources. It is hypothesized that powerful stellar winds generate the radio emission in S106 IR and CRL 961, in view of their miniscule 5-GHz angular size, strong 4.05 micron Br-alpha H-recombination line, and proximity to the centers of expanding molecular or ionized gas. All of the objects studied are sufficiently hot and active to produce ionizing radiation and/or powerful stellar winds. The disruption of the star-forming molecular cloud is in progress. The direct observation of high velocity molecular and ionized gas shows that energetic mass outflow is a major process associated with the birth and early life of the stars studied.
Bally John
Predmore Read
No associations
LandOfFree
Ionized gas in active molecular cloud cores does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Ionized gas in active molecular cloud cores, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ionized gas in active molecular cloud cores will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1305843