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http://dspace.mediu.edu.my:8181/xmlui/handle/10261/3714Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.creator | Barcons, Xavier | - |
| dc.date | 2008-04-24T01:34:14Z | - |
| dc.date | 2008-04-24T01:34:14Z | - |
| dc.date | 2007-11-30 | - |
| dc.date.accessioned | 2017-01-31T01:03:24Z | - |
| dc.date.available | 2017-01-31T01:03:24Z | - |
| dc.identifier | arXiv:0711.4888v1 [astro-ph] | - |
| dc.identifier | Astron. Nachr. / AN 999, No. 88, 789 – 792 (2006) | - |
| dc.identifier | http://dx.doi.org/10.1002/asna.200710893 | - |
| dc.identifier | 0004-6337 | - |
| dc.identifier | http://hdl.handle.net/10261/3714 | - |
| dc.identifier | 10.1002/asna.200710893 | - |
| dc.identifier.uri | http://dspace.mediu.edu.my:8181/xmlui/handle/10261/3714 | - |
| dc.description | Proceedings of the "XMM-Newton: the next decade", to appear in Astronomische Nachrichten. | - |
| dc.description | At low redshift (z<2), almost half of the baryons in the Universe are not found in bound structures like galaxies and clusters and therefore most likely reside in a Warm-Hot Intergalactic Medium (WHIM), as predicted by simulations. Attempts to detect WHIM filaments at cosmological distances in absorption towards bright background sources have yielded controversial results that I review here. I argue that a secure detection of absorption features by the WHIM is at the limit of the XMM-Newton capabilities, but feasible. A proper characterisation of the whole WHIM belongs to the realm of future X-ray missions. | - |
| dc.description | Financial support for this work has been provided by the Spanish Ministry of Education and Science under project ESP2006-13608-C02-01. | - |
| dc.description | Peer reviewed | - |
| dc.format | 76501 bytes | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.relation | Preprint | - |
| dc.rights | openAccess | - |
| dc.subject | Galaxies: intergalactic medium | - |
| dc.subject | Quasars: absorption lines | - |
| dc.subject | Astrophysics | - |
| dc.title | Searching for the Missing Baryons in the Warm-Hot Intergalactic Medium | - |
| dc.type | Pre-print | - |
| Appears in Collections: | Digital Csic | |
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