IRAS observations of two early-type pre-main-sequence stars in the association Chamaeleon I

Details IRAS observations of two early-type pre-main-sequence stars in the association Chamaeleon I IRAS observations of two early-type pre-main-sequence stars in the association Chamaeleon I

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...278l..37w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 278, March 1, 1984, p. L37-L39.

Astronomy and Astrophysics

Astronomy

14

Early Stars, Infrared Astronomy, Pre-Main Sequence Stars, Reflection Nebulae, Spaceborne Astronomy, Astronomical Maps, Cosmic Dust, Far Infrared Radiation, Stellar Envelopes, Supermassive Stars

Scientific paper

The most massive stars in the Chamaeleon I dark cloud, HD 97048 (A0 pe) and HD 97300 (A0 V), both associated with prominent reflection nebulae, were observed by IRAS at 50 and 100 μm, with 1arcmin.2 resolution. Both stars show large far-infrared fluxes from circumstellar dust and material in the reflection nebulae. At least one other source is embedded within the Cha I cloud close to HD 97300.

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