UBV photometry of IRAS 18062+2410 (Arkhipova+, 1999)

Details UBV photometry of IRAS 18062+2410 (Arkhipova+, 1999) UBV photometry of IRAS 18062+2410 (Arkhipova+, 1999)

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..90250030a&link_type=abstract

VizieR On-line Data Catalog: J/PAZh/25/30. Originally published in: 1999PAZh...25...30A; 1999AstL...25...25A

Other

Infrared Sources, Nebulae: Planetary, Photometry: Ubv, Spectroscopy

Scientific paper

The photometric and spectroscopic observations of IRAS 18062+2410 = V886 Her, a candidate for protoplanetary objects, in 1996-1997 are presented. The star exhibits rapid light variations with an amplitude up to 0.3mag in V. A high-resolution spectrum of IRAS shows absorption lines of H, HeI, OI, FeII, SiII, NaI and other species, including [OII], [NII], and [FeII] that belong to the stellar envelope. (1 data file).

Affiliated with

Also associated with

No associations

Rating

UBV photometry of IRAS 18062+2410 (Arkhipova+, 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 UBV photometry of IRAS 18062+2410 (Arkhipova+, 1999), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV photometry of IRAS 18062+2410 (Arkhipova+, 1999) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1824864