Issue |
A&A
Volume 421, Number 1, July I 2004
|
|
---|---|---|
Page(s) | 295 - 303 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361:20034193 | |
Published online | 11 June 2004 |
An atmospheric model for UZ Librae from mean Hα-line profiles
1
Astrophysikalisches Institut Potsdam (AIP), An der Sternwarte 16, 14482, Germany e-mail: kstrassmeier@aip.de
2
SAO, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MA 02138, USA e-mail: avrett@cfa.harvard.edu
Corresponding author: M. Zboril, mzboril@aip.de
Received:
14
August
2003
Accepted:
25
March
2004
We present the results from fitting a semi-empirical atmospheric
model including a chromosphere and a transition region to the mean
(seasonal) Balmer Hα line profiles of the RS CVn-type
K0-giant UZ Librae. As a first step, a static 1D spherical model was
applied to the mean component of the Hα-emission core and
its profile. The main result of the fitting is that the transition
region begins at a log mass depth of -1.8 g cm-2 at a temperature of 7400 K (approximately
3000 K warmer than the photosphere) and then has a steep increase
to the peak temperature of ≈106 K. A
stellar model in plane-parallel mode with
“partial-frequency redistribution” option in the line transfer
gave roughly the best fit. Subsequently, two-Gaussian
fitting of the phase-dependent Hα-line profiles yields a
complex velocity field. The radial velocities, from both the
absorption reversal and the main emission component, display
rotational and/or orbital modulation. The largest differences
between consecutive line profiles occur mostly in the red line
wings, suggesting the existence of both an inward-pointed
velocity field and sporadic radiation events possibly related to
flares. The total Hα emission, as derived from the
equivalent width, possibly also displays rotational modulation.
Indirect evidence is presented for the existence of circumstellar
matter in form of an Hα absorption shell. Finally, a
preliminary elemental abundance analysis suggests sub-solar
metallicity of dex based on ATLAS models, or -0.7 dex based on PHOENIX models.
Key words: stars: late-type / stars: activity / stars: atmospheres / stars: chromospheres / stars: individual: UZ Lib
© ESO, 2004
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