DY Per: Extremely Cool Galactic RCB Star?

Details DY Per: Extremely Cool Galactic RCB Star? DY Per: Extremely Cool Galactic RCB Star?

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..391...49z&link_type=abstract

Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, at Eberhard

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations of the extremely cool RCB candidate, DY Per, are presented
to specify its fundamental parameters and evolutionary status. CCD BVRI
photometry and spectroscopy was carried out in 2002/2004. A qualitative
analysis was made relative to the typical carbon stars of various types.

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