No CrossRef data available.
Article contents
Chandra Observations of The Antennae Galaxies (NGC 4038/39)
Published online by Cambridge University Press: 13 May 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
A deep (∼ 70ks) Chandra ACIS pointing at the merging system NGC 4038/39 gives us an exceptional detailed view of its X-ray emission and demonstrates the capabilities of Chandra's sub-arcsecond resolution. We detect an extraordinarily luminous population of pointlike sources, that may suggest 10-100M⊙ Black Hole counterparts. We also detect a luminous hot ISM, with features ranging to large scale outflows to hot superbubbles.
- Type
- The Inner Regions of Galaxies
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2001
References
Fabbiano, G.
1995a, in ‘X-Ray Binaries’, Lewin, W. H. G., van Paradijs, J., van den Heuvel, E. P. J., eds., Cambridge Astrophysics Series (Cambridge: University Press), p. 390.Google Scholar
Sansom, A.E., Dotani, T., Okada, K., Yamashita, A., & Fabbiano, G.
1996, MNRAS, 281, 48.Google Scholar
You have
Access