Chandra Observations of Embedded Young Stellar Objects

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dc.creatorKoyama, Katsuji
dc.date2001-09-19
dc.date.accessioned2026-07-07T02:00:04Z
dc.date.available2026-07-07T02:00:04Z
dc.descriptionThis paper reviews the Chandra deep exposure observations of star forming regions, rho-Ophiuchi, Orion Molecular Clouds 2 and 3, Sagittarius B2 and Monoceros R2. The results are; (1) class I protostars are found to exhibit higher temperature plasma than those of T Tauri stars, (2) heavily absorbed X-rays are discovered from the candidates of class 0 protostars, (3) hard and highly variable X-rays are observed from high-mass young stars, and (4) young brown dwarfs emit X-rays similar to those of low-mass young stars.
dc.description12 pages, 4 figures, to appear in the proceedings of the "Stellar Coronae in the Chandra and XMM-Newton Era", ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0109307
dc.identifierhttp://arxiv.org/abs/astro-ph/0109307
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3346
dc.subjectAstrophysics
dc.titleChandra Observations of Embedded Young Stellar Objects
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