Astronomy and Astrophysics – Astronomy
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..318s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 318-343.
Astronomy and Astrophysics
Astronomy
36
H Ii Regions, Infrared Astronomy, Molecular Clouds, Star Formation, Carbon Monoxide, Near Infrared Radiation, Pre-Main Sequence Stars, Spatial Resolution
Scientific paper
The results of a near-IR survey of the NGC 6334 massive H II region/molecular cloud region are presented. No widespread population of embedded stars is found in the cloud within the sensitivity limit. Three new possible premain-sequence objects are found. The mapping of near-IR extended emission is shown to be invaluable in pinpointing obscured H II regions. The locations of the youngest objects in NGC 6334 relative to evolved high-mass objects and H II regions show a likely causal link involving stellar winds or ionizing radiation, in the initiation of star formation.
Hyland A. R.
Straw Steven M.
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