The XMM-Newton Optical Monitor survey of the Taurus molecular cloud

2006/11/12 by M. Audard, Marc Audard, K. R. Briggs +11 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Cloud computing #Interstellar cloud #Molecular absorption #Molecular cloud #Optical depth #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066320

published as Astron.Astrophys.468:379-390,2007 · Accepted by A&A, to appear in a special section/issue dedicated to the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST). Version with higher resolution figures available at this http://www.issibern.ch/teams/Taurus/papers.html

arxiv created 2006/11/12 · openalex publication_date 2006/12/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context.The Optical Monitor (OM) on-board XMM-Newton obtained optical/ultraviolet data for the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), simultaneously with the X-ray detectors.

Citations

• The first high-resolution X-ray spectrum of a Herbig star: AB Aurigae
• X-ray emission from the young brown dwarfs of the Taurus molecular cloud
• A Simultaneous Optical and X‐Ray Variability Study of the Orion Nebula Cluster. I. Incidence of Time‐correlated X‐Ray/Optical Variations
• X-rays from jet-driving protostars and T Tauri stars
• High-resolution X-ray spectroscopy of T Tauri stars in the Taurus-Auriga complex
• Flares observed with XMM-Newton and the VLA
• The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
• Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton
• Relationship between X-ray and ultraviolet emission of flares from dMe stars observed by XMM-Newton

Cited by

• X-rays from T Tauri: a test case for accreting T Tauri stars