J/A+A/526/A44       Observations of II Peg                   (Lindborg+, 2011)

Doppler images of the RS Canum Venaticorum binary II Pegasi during the years 1994-2002. Lindborg M., Korpi M.J., Hackman T., Tuominen I., Ilyin I., Piskunov N. <Astron. Astrophys. 526, A44 (2011)> =2011A&A...526A..44L 2011A&A...526A..44L
ADC_Keywords: Stars, variable ; Spectroscopy Keywords: stars: individual: HD 224085 - stars: activity - stars: imaging - starspots Abstract: We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. The six maps from 1999-2002 are based on previously unpublished observations. Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. Description: The observations were collected with the SOFIN spectrograph at the Nordic Optical Telescope. The temperature maps were calculated using a Doppler imaging code based on Tikhonov regularization. Objects: -------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------- 23 55 04.1 +28 38 01 II Peg = HD 224085 -------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 27 144 Summary of the observations 1994-1995, 1996-1998, and 1999-2002 -------------------------------------------------------------------------------- See also: J/A+A/334/863 : II Peg radial velocities (Berdyugina+ 1998) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.6 d HJD Heliocentric Julian date 16- 23 F8.6 --- Phase Phase calculated based on the ephemeris given in the paper 25- 27 I3 --- S/N Signal-to-Noise Ratio -------------------------------------------------------------------------------- Acknowledgements: Marjaana Lindborg, marjaana.lindborg(at)helsinki.fi
(End) Patricia Vannier [CDS] 16-Nov-2010
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