The soft X-ray emission in direction of Hyades
- Author(s)
- P Mendes, Michael J. Freyberg, Dieter Breitschwerdt
- Abstract
It has been known for decades that the Local Bubble (LB) is a very important contributor to the diffuse soft x-ray background. The exact contribution of the LB in different directions of the sky is still unknown. With the advent of the new generation of x-ray satellites, like XMM-Newton and Chandra, we can performed on a systematic study of the spatial structure of the LB. We present a spectral study of the LB contribution to the soft x-ray background emission in the direction of Hyades and Ophiuchus.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Max-Planck-Institut für extraterrestrische Physik
- Journal
- European Space Agency, Special publications: ESA - SP
- Volume
- 1
- Pages
- 371-372
- No. of pages
- 2
- ISSN
- 0379-6566
- Publication date
- 2006
- Austrian Fields of Science 2012
- 103003 Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/ed2f643f-1501-4173-8ecf-12dd393035c2