Issue |
A&A
Volume 431, Number 3, March I 2005
|
|
---|---|---|
Page(s) | 1019 - 1026 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361:20042013 | |
Published online | 16 February 2005 |
The K-band intensity profile of R Leonis probed by VLTI/VINCI *
1
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany e-mail: mwittkow@eso.org
2
Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
3
Institut für Theoretische Astrophysik der Universität Heidelberg, Albert-Ueberle-Str. 2, 69120 Heidelberg, Germany
4
School of Physics, University of Sydney, NSW 2006, Australia
5
Research School for Astronomy and Astrophysics, Australian National University, Canberra, ACT 2600, Australia
Received:
15
September
2004
Accepted:
19
October
2004
We present near-infrared K-band interferometric measurements
of the Mira star R Leonis obtained in April 2001 and January 2002
with the VLTI, the commissioning instrument VINCI,
and the two test siderostats. These epochs correspond to near-maximum
stellar variability phases ~0.08 and ~1.02 (one cycle later),
respectively. The April 2001 data cover a range of spatial
frequencies (31–35 cycles/arcsecond) within the first
lobe of the visibility function. These measurements indicate
a center-to-limb intensity variation (CLV) that is clearly different
from a uniform disk (UD) intensity profile. We show that
these measured visibility values are consistent with predictions from recent
self-excited dynamic Mira model atmospheres that
include molecular shells close to continuum-forming layers.
We derive high-precision Rosseland diameters
of mas and
mas for the April 2001 and
January 2002 data, respectively. Together with literature estimates of the
distance and the bolometric flux, these values
correspond to linear radii of
and
, and to effective temperatures
of
K and
K, respectively.
Key words: techniques: interferometric / stars: late-type / stars: AGB and post-AGB / stars: atmospheres / stars: fundamental parameters / stars: individual: R Leo
© ESO, 2005
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