Measurements of Br-gamma and H2 in young stellar objects

Details Measurements of Br-gamma and H2 in young stellar objects Measurements of Br-gamma and H2 in young stellar objects

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aj....100.1244c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 100, Oct. 1990, p. 1244-1247.

Astronomy and Astrophysics

Astronomy

28

Emission Spectra, H Lines, Stellar Luminosity, Stellar Spectra, Bromine, Hydrogen Recombinations, Optical Thickness

Scientific paper

Measurements of emission-line fluxes for Br-gamma and H2 1-0 S(1) are presented for 30, mostly low-luminosity, young stellar objects. The strong hydrogen recombination lines in the low-luminosity objects are more difficult to explain than those in high-luminosity young stellar objects. A spectrum of the high-order Pfund emission lines (Pf 20-25) in S106-IRS3 is presented which indicates high optical depths in the Pfund lines in this source.

Affiliated with

Also associated with

No associations

Rating

Measurements of Br-gamma and H2 in young stellar objects 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 Measurements of Br-gamma and H2 in young stellar objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurements of Br-gamma and H2 in young stellar objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1301621