Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

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



ID: 661088.0, MPI für Astronomie / Publikationen_mpia
A study of heating and cooling of the ISM in NGC 1097 with Herschel-PACS and Spitzer-IRS
Authors:Beirão, P.; Armus, L.; Helou, G.; Appleton, P. N.; Smith, J.-D.; Croxall, K. V.; Murphy, E. J.; Dale, D. A.; Draine, B. T.; Wolfire, M. G.; Sandstrom, K. M.; Aniano, G.; Bolatto, A. D.; Groves, B.; Brandl, B. R.; Schinnerer, E.; Crocker, A. F.; Hinz, J. L.; Rix, H. -. W.; Kennicutt, R. C.; Calzetti, D.; Gil de Paz, A.; Dumas, G.; Galametz, M.; Gordon, K. D.; Hao, C. -. N.; Johnson, B.; Koda, J.; Krause, O.; van der Laan, T.; Leroy, A. K.; Li, Y.; Meidt, S. E.; Meyer, J. D.; Rahman, N.; Roussel, H.; Sauvage, M.; Srinivasan, S.; Vigroux, L.; Walter, F.; Warren, B. E.
Date of Publication (YYYY-MM-DD):2012
Journal Abbrev.:The Astrophysical Journal
Volume:751
Issue / Number:2
Start Page:id. 144
Audience:Not Specified
Abstract / Description:NGC 1097 is a nearby Seyfert 1 galaxy with a bright circumnuclear starburst ring, a strong large-scale bar, and an active nucleus. We present a detailed study of the spatial variation of the far-infrared (FIR) [C II]158 μm and [O I]63 μm lines and mid-infrared H2 emission lines as tracers of gas cooling, and of the polycyclic aromatic hydrocarbon (PAH) bands as tracers of the photoelectric heating, using Herschel-PACS and Spitzer-IRS infrared spectral maps. We focus on the nucleus and the ring, and two star-forming regions (Enuc N and Enuc S). We estimated a photoelectric gas heating efficiency ([C II]158 μm+[O I]63 μm)/PAH in the ring about 50% lower than in Enuc N and S. The average 11.3/7.7 μm PAH ratio is also lower in the ring, which may suggest a larger fraction of ionized PAHs, but no clear correlation with [C II]158 μm/PAH(5.5-14 μm) is found. PAHs in the ring are responsible for a factor of two more [C II]158 μm and [O I]63 μm emission per unit mass than PAHs in the Enuc S. spectral energy distribution (SED) modeling indicates that at most 25% of the FIR power in the ring and Enuc S can come from high-intensity photodissociation regions (PDRs), in which case G 0 ~ 102.3 and n H ~ 103.5 cm-3 in the ring. For these values of G 0 and n H, PDR models cannot reproduce the observed H2 emission. Much of the H2 emission in the starburst ring could come from warm regions in the diffuse interstellar medium that are heated by turbulent dissipation or shocks. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
Free Keywords:galaxies: individual: NGC 1097; galaxies: ISM; galaxies: starburst; infrared: galaxies
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://cdsads.u-strasbg.fr/abs/2012ApJ...751..144B
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.