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Home Search Quick Search Advanced Fulltext Browse Collections Persons My eDoc Session History Login Name: Password: Documentation Help Support Wiki Direct access to document ID:	Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents   history ID: 559069.0, MPI für Astronomie / Publikationen_mpia Far-infrared line imaging of the starburst ring in NGC 1097 with the Herschel/PACS spectrometer Authors: Beirão, P.; Armus, L.; Appleton, P. N.; Smith, J. D. T.; Croxall, K. V.; Murphy, E. J.; Dale, D. A.; Helou, G.; Kennicutt, R. C.; Calzetti, D.; Bolatto, A. D.; Brandl, B. R.; Crocker, A. F.; Draine, B. T.; Dumas, G.; Engelbracht, C. W.; Gil de Paz, A.; Gordon, K. D.; Groves, B.; Hao, C. N.; Hinz, J. L.; Hunt, L. K.; Johnson, B. D.; Koda, J.; Krause, O.; Leroy, A. K.; Meidt, S. E.; Richer, J.; Rix, H. W.; Rahman, N.; Roussel, H.; Sandstrom, K. M.; Sauvage, M.; Schinnerer, E.; Skibba, R. A.; Srinivasan, S.; Walter, F.; Warren, B. E.; Wilson, C. D.; Wolfire, M. G.; Zibetti, S. Language: English Date of Publication (YYYY-MM-DD): 2010 Title of Journal: Astronomy and Astrophysics Journal Abbrev.: A&A Volume: 518 Start Page: id.L60 Review Status: Peer-review Audience: Experts Only Abstract / Description: 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 μm, [OIII] 88 μm, [NII] 122 μm, [CII] 158 μm and [NII] 205 μm. We observe that in the [OI] 63 μm, [OIII] 88 μm, and [NII] 122 μm 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 ~220 km s-1 (inclination uncorrected) measured in all lines. The [OI] 63 μm/[CII] 158 μm 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 μm and [OIII] 88 μm maps. Variations of the [NII] 122 μm/[NII] 205 μm ratio correspond to a range in the ionized gas density between 150 and 400 cm-3. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. Free Keywords: photon-dominated region; infrared: galaxies; galaxies: Seyfert; galaxies: starburst; techniques: imaging spectroscopy; galaxies: individual: NGC 1097 External Publication Status: published Document Type: Article Communicated by: N. N. Affiliations: MPI für Astronomie Identifiers: URL:http://adsabs.harvard.edu/abs/2010A%26A...518L..60... [ID No:1] The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.