Superhumps in V1141 Aquilae

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

The results of the CCD observations of the 2002 superoutburst of V1141 Aql are described. We have detected clear superhumps characterized by the period of 0.05930(5) days. There was another, much weaker, modulation in the light curve of V1141 Aql. Its amplitude is equal to $0.012\pm0.002$ mag and its period to 0.03923(8) days. We have also discovered quasi periodic oscillations (QPOs) with a mean period equal to 130 s and amplitude of $0.025\pm0.004$ mag.
submitted to Acta Astronomica, 11 pages, 8 figures

Keywords

Astrophysics

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/5766

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0302379
 http://arxiv.org/abs/astro-ph/0302379

Collections

arXiv