Analysis of obscured infrared objects. IV - GL 490 and GL 2591

Details Analysis of obscured infrared objects. IV - GL 490 and GL 2591 Analysis of obscured infrared objects. IV - GL 490 and GL 2591

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231..736t&link_type=abstract

Astrophysical Journal, Part 1, vol. 231, Aug. 1, 1979, p. 736-741.

Astronomy and Astrophysics

Astrophysics

42

Infrared Spectra, Protostars, Stellar Evolution, Extremely High Frequencies, H Ii Regions, Hydrogen, Line Spectra

Scientific paper

Moderate-resolution spectra in the K band of two infrared objects (GL 490 and GL 2591) have been obtained. Hydrogen emission in the B-gamma line has been observed in GL 490 but not in GL 2591. In the case of GL 490, this observation indicates that the ultraviolet luminosity derived from the line emission is higher than expected from a ZAMS star of the same luminosity; however, the total ultraviolet luminosity is a small fraction of the total luminosity. A possible model for GL 2591 is presented which accounts for the presence of an infrared source and an H II region in close proximity with no detected hydrogen emission from the infrared source. This model assumes that GL 2591 is just beginning to dissipate its surrounding dust cloud.

Affiliated with

Also associated with

No associations

Rating

Analysis of obscured infrared objects. IV - GL 490 and GL 2591 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 Analysis of obscured infrared objects. IV - GL 490 and GL 2591, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of obscured infrared objects. IV - GL 490 and GL 2591 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1483507