Near-Infrared and Visual Photometry of the Mira Variables V Tau and X AUR

Details Near-Infrared and Visual Photometry of the Mira Variables V Tau and X AUR Near-Infrared and Visual Photometry of the Mira Variables V Tau and X AUR

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...190.2605h&link_type=abstract

American Astronomical Society, 190th AAS Meeting, #26.05; Bulletin of the American Astronomical Society, Vol. 29, p.810

Astronomy and Astrophysics

Astronomy

Scientific paper

We have been using a system of narrow-band, near-infrared filters to monitor changes in the infrared continuum magnitude and spectral type of several Mira variables (Rebel and Henson 1996, Bull. A.A.S., 28, 1399). Observations in V were added to the program at the beginning of 1997. We are now building simultaneous visual and near-infrared light curves with corresponding spectral type and color index variations. A comparison of the visual and infrared behavior will allow us to determine whether peculiarities in the visual light curves for these stars can be attributed to differential line blanketing effects or the phasing of temperature and diameter variations. Curves for a complete cycle of the short period Miras, V Tau and X Aur, are presented and the results discussed.

Affiliated with

Also associated with

No associations

Rating

Near-Infrared and Visual Photometry of the Mira Variables V Tau and X AUR 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 Near-Infrared and Visual Photometry of the Mira Variables V Tau and X AUR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near-Infrared and Visual Photometry of the Mira Variables V Tau and X AUR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-830896