X-ray emission from the young brown dwarfs of the Taurus molecular cloud

2006/08/25 by N. Grosso, K. R. Briggs, M. Guedel +13 · 2 citations
Physics and Astronomy · #Astrobiology #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Brown dwarf #Cloud computing #Computer science #Molecular cloud #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065559

published as Astron.Astrophys.468:391-403,2007 · 20 pages and 19 Figures. Accepted by A&A, to appear in a special section/issue dedicated to the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST). Preprint with higher resolution figures is available at http://hal.ccsd.cnrs.fr/ccsd-00090499

openalex publication_date 2006/08/25 · arxiv created 2006/08/31 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We report the X-ray properties of young (~3 Myr) bona fide brown dwarfs of the Taurus Molecular Cloud (TMC).

Citations

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• The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
• X-ray emission from a brown dwarf in the Pleiades
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• Are Coronae of Late‐Type Stars Made of Solar‐like Structures? The X‐Ray Surface Flux versus Hardness Ratio Diagram and the Pressure‐Temperature Correlation
• Relationship between X-ray and ultraviolet emission of flares from dMe stars observed by XMM-Newton

Cited by

• A statistical analysis of X-ray variability in pre-main sequence objects of the Taurus molecular cloud
• The first high-resolution X-ray spectrum of a Herbig star: AB Aurigae