Journal article
Star formation efficiency along the radio jet in Centaurus A
- Abstract:
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NGC 5128 (also known as Centaurus A) is the most nearby powerful AGN, widely studied at all wavelengths. Molecular gas has been found in the halo at a distance of ~ 20 kpc from the galaxy center, associated with H I shells, through CO line detection at SEST (Charmandaris et al. 2000, A&A, 356, L1). The molecular gas lies inside some IR and UV bright star-forming filaments that have recently been observed in the direction of the radio jets. These archival data from GALEX (FUV) and Herschel (IR...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, 3.9MB, Terms of use)
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- Publisher copy:
- 10.1051/0004-6361/201526409
Authors
Bibliographic Details
- Publisher:
- EDP Sciences
- Journal:
- Astronomy and Astrophysics More from this journal
- Volume:
- 586
- Article number:
- A45
- Publication date:
- 2016-01-25
- Acceptance date:
- 2015-11-17
- DOI:
- EISSN:
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1432-0746
- ISSN:
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0004-6361
Item Description
- Language:
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English
- Keywords:
- Pubs id:
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993331
- Local pid:
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pubs:993331
- Deposit date:
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2020-04-29
Terms of use
- Copyright holder:
- ESO
- Copyright date:
- 2016
- Rights statement:
- © ESO, 2016
- Notes:
- Note: an erratum exists for this article, originally published and available at: https://www.aanda.org/10.1051/0004-6361/201526409e
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