Dust Formation in the SC-type Star UY Cen

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

In February of 2002, the unassuming, small amplitude variable star UY Cen was observed by AAVSO astronomer Colin Henshaw in Oman to have vanished from the sky. Upon further observation, Henshaw and other AAVSO observers found the star had faded by more than two magnitudes. A historical study using prior published and unpublished observations, including those of archival photographic plates, and an analytical study of UY Cen was carried out during the summer of 2003. The primary results are presented here. Prior publications have classified UY Cen in the range of M-, C-, S-, and SC- type with little agreement. Closer analysis of recent spectroscopic data pinpointed the unique absorption features (ZrO, TiO, Na D) to be those of an SC-type star. Being that there are less than thirty confirmed or suspected SC-type stars, this classification raises more questions than it answers. Has UY Cen gone into decline before? Can we expect this sort of behavior from other SC-type stars, or if not, what makes UY Cen special compared with other stars of this class? Upon analysis of over one hundred photographic plates dating back to 1890 in the Harvard College Observatory plate archive, we can conclude that UY Cen has gone into decline at least once in the last century. Analysis of infrared data taken prior to and during the decline suggests dust formation. However, photometric data taken before the decline fitted with a black body curve shows no infrared excess prior to decline. Comparison of UY Cen to other SC-type stars showed no distinguishing characteristics other than the decline of 2002. This first analysis only partly answered our questions; there still remain many more questions to be answered of this unusual star. This project was supported by the NSF/REU grant AS T-0097694 and the Nantucket Maria Mitchell Association.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Dust Formation in the SC-type Star UY Cen 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 Dust Formation in the SC-type Star UY Cen, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust Formation in the SC-type Star UY Cen will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1421608

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.