Secular evolution in Mira variable pulsations Virtual Observatory Resource

Authors

1. Templeton M.R.
2. Mattei J.A.
3. Willson L.A.

Published by

CDS

Abstract

In this paper we present the results of our study of period change in 547 Mira variables using data from the AAVSO (American Association of Variable Star Observers). We use wavelet analysis to measure the period changes in individual Mira stars over the span of available data. By making linear fits to the period versus time measurements, we determine the average rates of period change, d(lnP)/dt, for each of these stars.

Keywords

1. Variable stars

Bibliographic source Bibcode

2005AJ....130..776T

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/130/776

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/130/776

Document Object Identifer DOI

doi:10.26093/cds/vizier.51300776

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/130/776
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/130/776
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/130/776

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/130/776/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/130/776/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/130/776/table1?