Issue |
A&A
Volume 366, Number 1, January IV 2001
|
|
---|---|---|
Page(s) | 178 - 196 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361:20000205 | |
Published online | 15 January 2001 |
δ Scuti and related stars: Analysis of the R00 Catalogue
1
Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
2
Institut für Astronomie, Universität Wien, Türkenschanzstr. 17, 1180, Austria
E. Rodríguez
Received:
21
September
2000
Accepted:
3
November
2000
We present a comprehensive analysis of the properties of the pulsating
δ Scuti and related variables based mainly on the content of the
recently published catalogue by Rodríguez et al. ([CITE],
hereafter R00). In particular, the primary observational properties such as
visual amplitude, period and visual
magnitude and the contributions from the Hipparcos, OGLE and MACHO long-term
monitoring projects are examined. The membership of these variables in open
clusters and multiple systems is also analyzed, with special
attention given to the δ Scuti pulsators situated in eclipsing binary
systems.
The location of the δ Scuti variables in the H-R diagram
is discussed on the basis of HIPPARCOS parallaxes and uvbyβ
photometry. New borders of the classical instability are presented.
In particular, the properties of the δ Scuti pulsators
with nonsolar surface abundances (SX Phe, λ Boo, ρ Pup,
δ Del and classical Am stars subgroups) are examined.
The Hipparcos parallaxes show that the available photometric
uvbyβ
absolute magnitude calibrations by Crawford can be applied correctly
to δ Scuti variables rotating faster than
100 km s
with normal
spectra. It is shown that systematic deviations
exist for the photometrically determined absolute magnitudes, which
correlate with
and
. The photometric
calibrations are found to fit the λ Boo stars,
but should not be used for the group of evolved metallic-line A stars.
The related γ Dor variables and the pre-main-sequence δ Scuti
variables are also discussed.
Finally, the variables catalogued with periods longer than 0
25 are
examined on a star-by-star basis in order to assign them to the proper
δ Scuti, RR Lyrae or γ Dor class.
A search for massive, long-period δ Scuti stars similar to
the triple-mode variable AC And is also carried out.
Key words: stars: variables: δ Scuti / stars: oscillations / stars: fundamental parameters
© ESO, 2001
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