Dust masses, compositions, and luminosities in the nuclear disks and the diffuse circumnuclear medium of Arp220
| dc.contributor.author | Dwek, Eli | |
| dc.contributor.author | Arendt, Richard | |
| dc.date.accessioned | 2020-09-11T16:07:12Z | |
| dc.date.available | 2020-09-11T16:07:12Z | |
| dc.date.issued | 2020-08-10 | |
| dc.description.abstract | We present an analysis of the 4-2600 μm spectral energy distributions (SEDs) of the west and east nuclei and the diffuse infrared (IR) region of the merger-driven starburst Arp 220. We examine several possible source morphologies and dust temperature distributions using a mixture of silicate and carbonaceous grains. From fits to the SEDs we derive dust masses, temperatures, luminosities, and dust inferred gas masses. We show that the west and east nuclei are powered by central sources deeply enshrouded behind ∼10²⁶ cm⁻² column densities of hydrogen with an exponential density distribution, and that the west and east nuclei are optically thick out to wavelengths of ∼1900 and ∼770 μm, respectively. The nature of the central sources cannot be determined from our analysis. We derive star formation rates or black hole masses needed to power the IR emission, and show that the [C II] 158μm line cannot be used as a tracer of the star formation rate in heavily obscured systems. Dust inferred gas masses are larger than those inferred from CO observations, suggesting either larger dust-to-H mass ratios, or the presence of hidden atomic H that cannot be inferred from CO observations. The luminosities per unit mass in the nuclei are ∼450, in solar units, smaller that the Eddington limit of ∼1000−3000 for an optically thick star forming region, suggesting that the observed gas outflows are primarily driven by stellar winds and supernova shock waves instead of radiation pressure on the dust. | en_US |
| dc.description.sponsorship | The research for this project was supported by NASA 16-ATP16-0004. We thank the referee for pointing out the detection of the [C II] emission in Arp 220 East, and for suggesting the discussion on the applicability of this line as a SFR tracer in heavily obscured systems. We also acknowledge helpful discussions with Jackie Fischer, Jason Glenn, and Nick Scoville. | en_US |
| dc.description.uri | https://iopscience.iop.org/article/10.3847/1538-4357/abad98 | en_US |
| dc.format.extent | 14 pages | en_US |
| dc.genre | journal articles | en_US |
| dc.identifier | doi:10.13016/m284ai-mldr | |
| dc.identifier.citation | Dwek, Eli, and Richard Arendt. Dust Masses, Compositions, and Luminosities in the Nuclear Disks and the Diffuse Circumnuclear Medium of Arp 220. The Astrophyiscal Journal 901 (Sept. 18, 2020), no. 1. https://iopscience.iop.org/article/10.3847/1538-4357/abad98. | |
| dc.identifier.uri | http://hdl.handle.net/11603/19637 | |
| dc.identifier.uri | https://doi.org/10.3847/1538-4357/abad98 | |
| dc.language.iso | en_US | en_US |
| dc.publisher | IOP | |
| dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
| dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
| dc.relation.ispartof | UMBC Physics Department | |
| dc.relation.ispartof | UMBC Faculty Collection | |
| dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | |
| dc.rights | Public Domain Mark 1.0 | * |
| dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | |
| dc.rights.uri | http://creativecommons.org/publicdomain/mark/1.0/ | * |
| dc.title | Dust masses, compositions, and luminosities in the nuclear disks and the diffuse circumnuclear medium of Arp220 | en_US |
| dc.type | Text | en_US |
| dcterms.creator | https://orcid.org/0000-0001-8403-8548 |