X-ray monitoring of optical novae in M 31 from July 2004 to February 2005

200784 citationsJournal Articlegreen Open Access

Authors

W. Pietsch · Max Planck Institute for Extraterrestrial Physics

F. Haberl · Max Planck Society

G. Sala · Max Planck Society

H. Stiele · Max Planck Society

K. Hornoch · Vitkovice - Research and Development (Czechia)

A. Riffeser · Max Planck Society

J. Fliri ·

Abstract

Context.Optical novae have recently been identified as the major class of supersoft X-ray sources in M 31 based on ROSAT and early XMM-Newton and Chandra observations.

Topics & Keywords

Astrophysical Phenomena and Observations Astrophysics and Cosmic Phenomena Pulsars and Gravitational Waves Research

Publication Details

Published in: Astronomy and Astrophysics

Volume 465, Issue 2, pp. 375-392

DOI: 10.1051/0004-6361:20066812

Field-Weighted Citation Impact: 7.46

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X-ray monitoring of optical novae in M 31 from July 2004 to February 2005

Authors

Abstract

Topics & Keywords

Publication Details