IRAS observations of the cool galactic hypergiants

Details IRAS observations of the cool galactic hypergiants IRAS observations of the cool galactic hypergiants

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985obs...105..229s&link_type=abstract

The Observatory, vol. 105, p. 229-232 (1985)

Physics

6

Scientific paper

IRAS observations of the galactic stars of spectral type later than F0 and with bolometric absolute magnitudes brighter than -8.0 have been added to the published ground-based photometry to search for thermal re-emission from dust resulting from mass loss. Only the stars cooler than early G exhibit substantial dust signatures among the objects in the present sample. The size of the 10-micron excess appears to be linked to the amount of general thermal re-emission.

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