Late-type stars toward galactic antirotation (Westpfahl+ 1999)

Details Late-type stars toward galactic antirotation (Westpfahl+ 1999) Late-type stars toward galactic antirotation (Westpfahl+ 1999)

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycat..71111169w&link_type=abstract

VizieR On-line Data Catalog: J/PASP/111/1169. Originally published in: 1999PASP..111.1169W

Computer Science

Stars: Late-Type, Photometry: Ubv, Mk Spectral Classification

Scientific paper

Low-resolution objective-prism spectra (1360{AA}/mm at H{gamma}) of 184 late-type stars in the Galactic antirotation direction have been obtained with the Curtis Schmidt telescope at Cerro Tololo Inter-American Observatory. The stars have been classified into three groups: F6-G2, G3-K0, and K1-M8. Subsequent observations on the BV and DDO systems have been obtained. The correlation between the thin-prism classes and the DDO classes is as expected, with no significant systematic differences of note. A comparison of Guide Star Catalog magnitudes, corrected to V, is also made, with favorable results. The stars in this list are expected to be useful for studying the structure and star formation history of the Milky Way.
(3 data files).

Affiliated with

Also associated with

No associations

Rating

Late-type stars toward galactic antirotation (Westpfahl+ 1999) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Late-type stars toward galactic antirotation (Westpfahl+ 1999), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Late-type stars toward galactic antirotation (Westpfahl+ 1999) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1546527