Spectroscopy of the brightest optical counterparts of X-ray sources in the direction of M 31 and M 33

2006/02/17 by D. Hatzidimitriou, W. Pietsch, Z. Misanovic +2 · 1 citation
Engineering · Physics and Astronomy · #Archaeology #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Context (archaeology) #Engineering #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geography #Local Group #Optics #Physics #Spectroscopy #Spiral (railway) #Spiral galaxy #Stellar, planetary, and galactic studies #X-ray #astro-ph

paper · pdf · doi:10.1051/0004-6361:20054402

9 pages, 12 figures, accepted in A&A

arxiv created 2006/02/17 · openalex publication_date 2006/05/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.Recent surveys of the Local Group spiral Galaxies M 31 and M 33 with XMM-Newton yielded a large number of X-ray sources.

Citations

• A Synoptic X‐Ray Study of M31 with theChandraHigh Resolution Camera
• An optimal extraction algorithm for CCD spectroscopy
• Some Like It Hot: The X‐Ray Emission of the Giant Star YY Mensae
• XMM-Newton survey of the Local Group galaxy M 33
• Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton
• The USNO-B Catalog

Cited by

• Spectroscopy of the bright optical counterparts of X-ray sources in the direction of M 31