Spectrophotometry of cool angular-diameter stars

Details Spectrophotometry of cool angular-diameter stars Spectrophotometry of cool angular-diameter stars

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...215..584h&link_type=abstract

Astrophysical Journal, Part 1, vol. 215, July 15, 1977, p. 584-596. NSF-supported research.

Astronomy and Astrophysics

Astronomy

25

Infrared Astronomy, Late Stars, Radiant Flux Density, Stellar Spectrophotometry, Atmospheric Scattering, Broadband, Diameters, Infrared Spectrophotometers, Photometry, Stellar Atmospheres, Stellar Luminosity

Scientific paper

Wide-band photometry and spectrophotometric scans are combined to obtain incident flux curves for 26 late-type stars. The wavelength range covered for most stars is from 0.4 to 3.0 microns with a typical resolution of approximately 200. Nineteen of these stars have published angular diameters, so that the emergent flux may be computed from the incident flux.

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