Journal
ASTRONOMY & ASTROPHYSICS
Volume 518, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201014592
Keywords
photon-dominated region; infrared: galaxies; galaxies: Seyfert; galaxies: starburst; techniques: imaging spectroscopy; galaxies: individual: NGC 1097
Categories
Funding
- NASA
- BMVIT (Austria)
- ESA-PRODEX (Belgium)
- CEA (France)
- DLR (Germany)
- ASI (Italy)
- CICT (Spain)
- MCT (Spain)
- CNES (France)
- Science and Technology Facilities Council [ST/H00243X/1] Funding Source: researchfish
Ask authors/readers for more resources
NGC 1097 is a nearby SBb galaxy with a Seyfert nucleus and a bright starburst ring. We study the physical properties of the interstellar medium (ISM) in the ring using spatially resolved far-infrared spectral maps of the circumnuclear starburst ring of NGC 1097, obtained with the PACS spectrometer on board the Herschel Space Observatory. In particular, we map the important ISM cooling and diagnostic emission lines of [OI] 63 mu m, [OIII] 88 mu m, [NII] 122 mu m, [CII] 158 mu m and [NII] 205 mu m. We observe that in the [OI] 63 mu m, [OIII] 88 mu m, and [NII] 122 mu m line maps, the emission is enhanced in clumps along the NE part of the ring. We observe evidence of rapid rotation in the circumnuclear ring, with a rotation velocity of similar to 220 km s(-1) (inclination uncorrected) measured in all lines. The [OI] 63 mu m/[CII] 158 mu m ratio varies smoothly throughout the central region, and is enhanced on the northeastern part of the ring, which may indicate a stronger radiation field. This enhancement coincides with peaks in the [OI] 63 mu m and [OIII] 88 mu m maps. Variations of the [NII] 122 mu m/[NII] 205 mu m ratio correspond to a range in the ionized gas density between 150 and 400 cm(-3).
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available