Distribution and studies of the infrared stellar population in the galaxy. IV - Baade's window spectroscopy

Details Distribution and studies of the infrared stellar population in the galaxy. IV - Baade's window spectroscopy Distribution and studies of the infrared stellar population in the galaxy. IV - Baade's window spectroscopy

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...95..379r&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 95, no. 2, p. 379-388.

Astronomy and Astrophysics

Astronomy

5

Astronomical Spectroscopy, Infrared Astronomy, Milky Way Galaxy, Star Distribution, Carbon Monoxide, Galactic Bulge, Infrared Photometry, Metallicity, Stellar Spectrophotometry, Water

Scientific paper

The clear Galactic area known as Baade's window is investigated by means of H2O and CO observations with an IR photometer spectrometer to statistically group the sample of objects. An intrinsic spread in the colors and CO and H2O indices of the sources is argued to cause the significant spread in the JHK diagram for this region. The stars with strong CO bands are interpreted as disk stars, and the CO-weak stars are considered Galactic bulge members.

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