Near-infrared photometry of late-type stars with balloon-borne telescope

Details Near-infrared photometry of late-type stars with balloon-borne telescope Near-infrared photometry of late-type stars with balloon-borne telescope

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977tokab.251.2889k&link_type=abstract

Tokyo Astronomical Observatory, Tokyo Astronomical Bulletin, Second Series, no. 251, Dec. 17, 1977, p. 2889-2893.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Infrared Astronomy, Infrared Photometry, Late Stars, Near Infrared Radiation, Balloon-Borne Instruments, Energy Distribution, Infrared Telescopes, K Stars, Stellar Magnitude

Scientific paper

Results are presented for balloon-borne near-IR (J H Omega K) photometry of 14 stars, including two A-type main-sequence comparison stars, one G9 III reference star, and 11 M- and K-type giants and supergiants. The telescope system used consisted of a 15-cm reflector and a PbS photometer. The overall energy-distribution pattern for 13 of the observed stars is plotted. A systematic trend is found whereby the gradient diminishes from early to late spectral type.

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