Infrared Excesses in the M Supergiants of H and χ Persei
1973; IOP Publishing; Volume: 186; Linguagem: Inglês
10.1086/181374
ISSN1538-4357
AutoresMartin Cohen, John E. Gaustad,
Tópico(s)Astrophysics and Star Formation Studies
Resumoview Abstract Citations (24) References (9) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Infrared Excesses in the M Supergiants of H and χ Persei Cohen, Martin ; Gaustad, John E. Abstract Infrared photometry from 3 to 18 microns has been obtained of the M supergiants in the young association h and Persei. A color excess indicative of silicate dust is observed for all stars, which correlates with higher luminosity and lower surface temperature. Subject headings: circumstellar shells - infrared - late-type stars - photometry Publication: The Astrophysical Journal Pub Date: December 1973 DOI: 10.1086/181374 Bibcode: 1973ApJ...186L.131C full text sources ADS | data products SIMBAD (41)
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