A deep XMM-Newton X-ray observation of the Chamaeleon I dark cloud

2006/09/26 by J. Robrade, J. H. M. M. Schmitt · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #Cloud computing #Herbig Ae/Be star #Ideal (ethics) #Main sequence #Molecular cloud #O-type star #Star (game theory) #Stars #T Tauri star #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066250

10 pages, 11 figures, accepted by A&A

openalex publication_date 2006/09/26 · arxiv created 2006/10/26 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.Low-mass stars are known to exhibit strong X-ray emission during the early stages of evolution. Nearby star forming regions are ideal targets to study the X-ray properties of pre-main sequence stars.

Citations

• X-ray accretion signatures in the close CTTS binary V4046 Sagittarii
• The Origin of T Tauri X‐Ray Emission: New Insights from the Chandra Orion Ultradeep Project
• The Two Micron All Sky Survey (2MASS)

Cited by

• ASPITZERSURVEY OF MID-INFRARED MOLECULAR EMISSION FROM PROTOPLANETARY DISKS. II. CORRELATIONS AND LOCAL THERMAL EQUILIBRIUM MODELS