UBV light curve and spectroscopy of StHa62 (Arkhipova+, 2006)

Details UBV light curve and spectroscopy of StHa62 (Arkhipova+, 2006) UBV light curve and spectroscopy of StHa62 (Arkhipova+, 2006)

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..90320737a&link_type=abstract

VizieR On-line Data Catalog: J/PAZh/32/737. Originally published in: 2006PAZh...32..737A; 2006AstL...32..661A

Astronomy and Astrophysics

Astronomy

Nebulae: Planetary, Photometry: Ubv, Spectroscopy

Scientific paper

Photoelectric observations of HD 51585 (OY Gem), a B[e] star with an infrared excess and a candidate for protoplanetary nebulae, obtained with a 60-cm telescope at the Crimean Station of Sternberg Astronomical Institute in 1992-2005 are presented. The star exhibited rapid irregular brightness variations with amplitudes from 0.1mag in the V band to 0.2mag in the U band within the observing season as well as slow systematic variations. with a quasi-period of ~2800-days. Low-resolution spectroscopy performed in 1994-2005 has revealed significant variability of the Balmer and Paschen hydrogen emission lines as well as the HeI and OI lines. Equivalent widths are given for the HI, HeI, OI, and FeII lines. Correlation has been found between the star's photometric variability and the hydrogen line intensities.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

UBV light curve and spectroscopy of StHa62 (Arkhipova+, 2006) 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 UBV light curve and spectroscopy of StHa62 (Arkhipova+, 2006), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV light curve and spectroscopy of StHa62 (Arkhipova+, 2006) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1361741