Broad-band 20-33-micron photometry of young stars

Details Broad-band 20-33-micron photometry of young stars Broad-band 20-33-micron photometry of young stars

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977aj.....82..725s&link_type=abstract

Astronomical Journal, vol. 82, Sept. 1977, p. 725-728.

Astronomy and Astrophysics

Astronomy

24

Early Stars, Infrared Spectra, Stellar Spectrophotometry, Broadband, Luminosity, Radiant Flux Density, Silicates, Stellar Evolution, Stellar Models, Stellar Temperature

Scientific paper

Broad-band flux measurements in the 20-33-micron spectral region are presented for 11 young stars, including Allen's (1972) source in NGC 2264, Cohen's (1973) source near the Rosette Nebula, and V1057 Cyg. All of the spectral energy distributions peak in the near-infrared and, except for the spectrum of V1057 Cyg, none show strong evidence of silicate bands at 20 microns. Allen's source is not resolved in multiaperture flux measurements at 20 and 33 microns, implying an upper limit on its angular diameter of 7 arcsec. The strength of the circumstellar 10- and 20-micron silicate emission features of V1057 Cyg had faded considerably by June 1974, but showed little change in observations continuing until September 1975.

Affiliated with

Also associated with

No associations

Rating

Broad-band 20-33-micron photometry of young 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 Broad-band 20-33-micron photometry of young stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Broad-band 20-33-micron photometry of young stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1092596