A Morphological Study of Infrared Line Emission in Compact Star-Forming Regions

Details A Morphological Study of Infrared Line Emission in Compact Star-Forming Regions A Morphological Study of Infrared Line Emission in Compact Star-Forming Regions

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aj....117.2448s&link_type=abstract

The Astronomical Journal, Volume 117, Issue 5, pp. 2448-2465.

Astronomy and Astrophysics

Astronomy

3

Ism: H Ii Regions, Ism: Individual (S61, S80), Ism: Individual: Alphanumeric: S83, Ism: Individual: Alphanumeric: S93, Ism: Individual: Alphanumeric: S99, Ism: Individual: Alphanumeric: S146, Ism: Individual: Alphanumeric: S148, Ism: Individual: Alphanumeric: S152, Ism: Individual: Alphanumeric: S156, Ism: Individual (S175, S186), Ism: Molecules, Infrared Radiation

Scientific paper

Near-infrared broadband and narrowband images are presented for 11 Galactic star-forming regions. Data were taken using the infrared camera on the Mount Palomar 60 inch (1.5 m) telescope with the broadband filters J, H, and K and with narrowband filters centered on H_2 and Brgamma. The morphologies of these regions are compared with ultraviolet fluorescence and shock front models of line emission. We find that the majority of these star-forming regions can be described by ultraviolet fluorescence.

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