Journal article
Polycyclic aromatic hydrocarbons in seyfert and star-forming galaxies
- Abstract:
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Polycyclic Aromatic Hydrocarbons (PAHs) are carbon-based molecules resulting from the union of aromatic rings and related species, which are likely responsible for strong infrared emission features. In this work, using a sample of 50 Seyfert galaxies (DL < 100 Mpc) we compare the circumnuclear (inner kpc) PAH emission of AGN to that of a control sample of star-forming galaxies (22 luminous infrared galaxies and 30 H ii galaxies), and investigate the differences betwe...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Accepted manuscript, 1.9MB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/stab3127
Authors
Bibliographic Details
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 509
- Issue:
- 3
- Pages:
- 4256–4275
- Publication date:
- 2021-10-29
- Acceptance date:
- 2021-10-22
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Language:
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English
- Keywords:
- Pubs id:
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1211603
- Local pid:
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pubs:1211603
- Deposit date:
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2021-11-22
Terms of use
- Copyright holder:
- García-Bernete et al.
- Copyright date:
- 2021
- Rights statement:
- © 2021 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
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