The near-infrared spectrum of the Herbig Ae-Be stars

Details The near-infrared spectrum of the Herbig Ae-Be stars The near-infrared spectrum of the Herbig Ae-Be stars

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...264..554l&link_type=abstract

Astrophysical Journal, Part 1, vol. 264, Jan. 15, 1983, p. 554-559.

Astronomy and Astrophysics

Astronomy

36

A Stars, B Stars, Emission Spectra, Herbig-Haro Objects, Infrared Astronomy, Stellar Spectra, Bremsstrahlung, Cosmic Dust, Near Infrared Radiation, Stellar Envelopes

Scientific paper

Near-infrared photometric data in the J, H, K, L, and M bands are presented for a sample of Ae-Be stars associated with nebulosity. The mechanism of the emission is examined, and the observational data are compared with theoretical models to account for the infrared excess. A model is developed to account for the observations in which the main source of IR emission is the bremsstrahlung from H2(-). Several exceptions, including LkH-alpha 198, R Mon, and LkH-alpha 233, are examined. It is found that two of the stars, BD plus 41.3731 degrees and LkH-alpha 215 do not show appreciable IR excess.

Affiliated with

Also associated with

No associations

Rating

The near-infrared spectrum of the Herbig Ae-Be stars 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 The near-infrared spectrum of the Herbig Ae-Be stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The near-infrared spectrum of the Herbig Ae-Be stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1195995