中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns??Based on Herschel observations. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

文献类型:期刊论文

作者Lu,Nanyao1,2,3; Zhao,Yinghe3,4,5,6; Díaz-Santos,Tanio7; Xu,C. Kevin1,2,3; Gao,Yu6; Armus,Lee8; Isaak,Kate G.9; Mazzarella,Joseph M.3; van der Werf,Paul P.10; Appleton,Philip N.3
刊名The Astrophysical Journal Supplement Series
出版日期2017-05-03
卷号230期号:1
ISSN号0067-0049
关键词galaxies: active galaxies: ISM galaxies: star formation infrared: galaxies ISM: molecules submillimeter: galaxies
DOI10.3847/1538-4365/aa6476
英文摘要Abstract We describe a Herschel Space Observatory 194–671 μm spectroscopic survey of a sample of 121 local luminous infrared galaxies and report the fluxes of the CO J to J–1 rotational transitions for , the [N ii] 205 μm line, the [C i] lines at 609 and 370 μm, as well as additional and usually fainter lines. The CO spectral line energy distributions (SLEDs) presented here are consistent with our earlier work, which was based on a smaller sample, that calls for two distinct molecular gas components in general: (i) a cold component, which emits CO lines primarily at J???4 and likely represents the same gas phase traced by CO (1?0), and (ii) a warm component, which dominates over the mid-J regime (4??10. The flux ratios of the two [C i] lines imply modest excitation temperatures of 15–30 K; the [C i] 370 μm line scales more linearly in flux with CO (4?3) than with CO (7?6). These findings suggest that the [C i] emission is predominantly associated with the gas component defined in (i) above. Our analysis of the stacked spectra in different far-infrared (FIR) color bins reveals an evolution of the SLED of the rotational transitions of vapor as a function of the FIR color in a direction consistent with infrared photon pumping.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0067-0049-230-1-AA6476
源URL[http://libir.pmo.ac.cn/handle/332002/23773]  
专题中国科学院紫金山天文台
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences (CAS), Beijing 100012, China; nanyao.lu@gmail.com
2.South American Center for Astronomy, CAS, Camino El Observatorio 1515, Las Condes, Santiago, Chile
3.Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA
4.Yunnan Observatories, CAS, Kunming 650011, China
5.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650011, China
6.Purple Mountain Observatory, CAS, Nanjing 210008, China
7.Nucleo de Astronomia de la Facultad de Ingenieria, Universidad Diego Portales, Av. Ejercito Libertador 441, Santiago, Chile
8.Spitzer Science Center, California Institute of Technology, MS 220-6, Pasadena, CA 91125, USA
9.Scientific Support Office, European Space Research and Technology Centre (ESA-ESTEC/SCI-S), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
10.Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands
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Lu,Nanyao,Zhao,Yinghe,Díaz-Santos,Tanio,et al. A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns??Based on Herschel observations. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.[J]. The Astrophysical Journal Supplement Series,2017,230(1).
APA Lu,Nanyao.,Zhao,Yinghe.,Díaz-Santos,Tanio.,Xu,C. Kevin.,Gao,Yu.,...&Surace,Jason A..(2017).A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns??Based on Herschel observations. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA..The Astrophysical Journal Supplement Series,230(1).
MLA Lu,Nanyao,et al."A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns??Based on Herschel observations. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.".The Astrophysical Journal Supplement Series 230.1(2017).

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