The recognition of late peculiar giants through photometry

Details The recognition of late peculiar giants through photometry The recognition of late peculiar giants through photometry

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...235..277h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 235, no. 1-2, Aug. 1990, p. 277-281.

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Giant Stars, Late Stars, Peculiar Stars, Cool Stars, Stellar Spectra, Stellar Spectrophotometry, Ubv Spectra

Scientific paper

Using broad-band photometry such as UBVRI or intermediate-band
photometry such as DOD, normal giants may be separated from peculiar
stars. This is of particular interest in the case of objects for which
normal spectroscopy is difficult to obtain.

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