2003/02/17 by A. Rodríguez-Ardila, A. Rodriguez-Ardila, S. M. Viegas +1 · 3 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Infrared #Luminosity #Luminous infrared galaxy #Physics #Quasar #Spectral line #Star formation #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2003.06538.x
5 pages, 1 figure. Accepted to MNRAS pink pages
arxiv created 2003/02/17 · openalex publication_date 2003/04/21 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We report the detection of the 3.3-μm polycyclic aromatic hydrocarbon (PAH) feature in two Seyfert 1 galaxies (NGC 3227 and Mrk 766) and one QSO (Mrk 478), observed with SpeX at the Infrared Telescope Facility at a spectral resolution not previously attained for these types of objects. Except for NGC 3227, this is the first time that the 3.3-μm PAH emission has been detected in Mrk 766 and 478. The widths of the emission, reported also for the first time, are rather similar, ranging from 450 to 550 Å. The luminosity of the 3.3-μm PAH emission measured in the QSO Mrk 478 places it at a level similar to that found in starburst and infrared-luminous galaxies, and implies that this object is having a vigorous burst of star formation. The spatial resolution of the spectra allows us to constrain the location of the star-forming region to the inner 1 kpc for the QSO and 150 pc for the Seyferts. Our results support the idea that these objects reside in molecular gas-rich galaxies and that their observed infrared excess is primarily due to star formation, as previously indicated by CO and H2 observations. We also report, for Mrk 1239, the presence of a broad emission feature centred at 3.43 μm, not previously detected in an extragalactic object and the origin of which is not yet clear.