|Reference : Chandra/ACIS observation of NGC 346|
|Scientific congresses and symposiums : Paper published in a book|
|Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics|
|Chandra/ACIS observation of NGC 346|
|Nazé, Yaël [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Sciences spatiales >]|
|Stevens, I. R. [U. Birmingham]|
|Hartwell, J. [U. Birmingham]|
|XMEGA Group, Collaboration [> > > >]|
|Bulletin of the American Astronomical Society|
|[en] The cluster NGC346 is the largest star formation region in the SMC. It contains a large fraction of the early-type O stars of this galaxy. In the outskirts of this cluster lies HD 5980, a unique system of massive stars of which one component underwent a LBV-type eruption in 1993. The XMEGA consortium has obtained one deep (100 ks) Chandra exposure of NGC 346. It shows ~70 point sources, of which only half possess an optical counterpart; strong emission from HD 5980; and diffuse emission associated with the cluster and SNR 0057-7226.|
There is no file associated with this reference.
All documents in ORBi are protected by a user license.