The detection of an IR excess toward the globular cluster RV Tauri variable M28 V17

Details The detection of an IR excess toward the globular cluster RV Tauri variable M28 V17 The detection of an IR excess toward the globular cluster RV Tauri variable M28 V17

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...346l..29n&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 346, Nov. 1, 1989, p. L29-L32.

Astronomy and Astrophysics

Astrophysics

9

Asymptotic Giant Branch Stars, Globular Clusters, Infrared Radiation, Planetary Nebulae, Variable Stars, Abundance, Color-Color Diagram, Metallicity, Stellar Envelopes, Stellar Evolution, Stellar Luminosity

Scientific paper

The paper presents the results of a search for IR emission excesses toward three globular cluster stars. Two of the stars are RV Tau variables (M28 V17 and M5 V85) and one is believed to be a W Vir variable (M5 V42) which is historically linked to the RV Tau class. Consideration is given to the implications of the observed detections, in particular, the establishment of M28 V17 as a star in a globular cluster that is indistinguishable from the Preston type A subclass.

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