High temporal resolution spectroscopic observations of UV Cet type flare stars

Details High temporal resolution spectroscopic observations of UV Cet type flare stars High temporal resolution spectroscopic observations of UV Cet type flare stars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.560..491c&link_type=abstract

Proceedings of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, held 5-9 July, 2004 in Hamburg, Germany.

Other

3

Stars: Activity, Stars: Chromospheres, Stars: Spectroscopy: Optical, Stars: Flare, Stars: Uv Cet Type, Stars: Late-Type

Scientific paper

We present the first results of a high temporal resolution spectroscopic monitoring of the UV Ceti-type flare stars EQ Vir, DK Leo, CR Dra, DT Vir, CE Boo, VV Lyn, DP Dra, V1054 Oph, AD Leo, BL Lyn and YZ CMi. The observations were done using the IDS spectrograph at the 2.5 m Isaac Newton Telescope (INT) of the El Roque de los Muchachos Observatory (La Palma, Canary Islands, Spain). Intermediate resolution spectra, including the Balmer series from Hβ to H11 as well as the He I λ4026 AA and the Ca II H & K lines, were taken using the R1200B dispersion grating (reciprocal dispersion of 0.48 AA/pixel). The great number of spectra taken each night with high temporal resolution (exposure times as short as 60 s) allows us to analyse the time evolution of the emission lines in order to identify flares. Other variations at different scales have been also observed. A comparison between all the observed stars have been done. Finally, for the strongest flares or changes, we study differences on the behaviour of the lines of interest.

Affiliated with

Also associated with

No associations

Rating

High temporal resolution spectroscopic observations of UV Cet type flare stars 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 High temporal resolution spectroscopic observations of UV Cet type flare stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High temporal resolution spectroscopic observations of UV Cet type flare stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1215335