Discovery of X-Ray Emission from Young Suns in the Small Magellanic Cloud
- Autor(en)
- Lidia M. Oskinova, W. Sun, C. J. Evans, V. Hénault-Brunet, Y.-H. Chu, J. S., III Gallagher, Mariela A. Guerrero, Robert A. Gruendl, M. Güdel, S. Silich, Yang Chen, Yaël Nazé, Rainer Hainich, J. Reyes-Iturbide
- Abstrakt
We report the discovery of extended X-ray emission within the young star
cluster NGC 602a in the Wing of the Small Magellanic Cloud (SMC) based
on observations obtained with the Chandra X-Ray Observatory. X-ray
emission is detected from the cluster core area with the highest stellar
density and from a dusty ridge surrounding the H II region. We use a
census of massive stars in the cluster to demonstrate that a cluster
wind or wind-blown bubble is unlikely to provide a significant
contribution to the X-ray emission detected from the central area of the
cluster. We therefore suggest that X-ray emission at the cluster core
originates from an ensemble of low- and solar-mass pre-main-sequence
(PMS) stars, each of which would be too weak in X-rays to be detected
individually. We attribute the X-ray emission from the dusty ridge to
the embedded tight cluster of the newborn stars known in this area from
infrared studies. Assuming that the levels of X-ray activity in young
stars in the low-metallicity environment of NGC 602a are comparable to
their Galactic counterparts, then the detected spatial distribution,
spectral properties, and level of X-ray emission are largely consistent
with those expected from low- and solar-mass PMS stars and young stellar
objects (YSOs). This is the first discovery of X-ray emission
attributable to PMS stars and YSOs in the SMC, which suggests that the
accretion and dynamo processes in young, low-mass objects in the SMC
resemble those in the Galaxy.
- Organisation(en)
- Institut für Astrophysik
- Externe Organisation(en)
- Instituto de Astrofísica de Andalucía, The Royal Observatory, Edinburgh, Universität Potsdam, Nanjing University, University of Edinburgh, University of Illinois at Urbana-Champaign, University of Wisconsin, Madison, National Institute of Astrophysics, Optics and Electronics (INAOE), Université de Liège, Universidade Estadual de Santa Cruz
- Journal
- The Astrophysical Journal: an international review of astronomy and astronomical physics
- Band
- 765
- Anzahl der Seiten
- 12
- ISSN
- 0004-637X
- DOI
- https://doi.org/10.1088/0004-637X/765/1/73
- Publikationsdatum
- 03-2013
- Peer-reviewed
- Ja
- ÖFOS 2012
- 103004 Astrophysik, 103003 Astronomie
- Schlagwörter
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/6b4424e7-a356-45d1-bced-cdf80f622c23