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.

doi:10.3847/1538-4365/aa6476

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	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.
	Lu,Nanyao 4,5,6; Zhao,Yinghe 3,6,7,8; Díaz-Santos,Tanio 9; Xu,C. Kevin 4,5,6; Gao,Yu 8; Armus,Lee 10; Isaak,Kate G.11; Mazzarella,Joseph M.6; van der Werf,Paul P.12; Appleton,Philip N.6
刊名	The Astrophysical Journal Supplement Series
	2017-05-03
卷号	230 期号:1
关键词	galaxies: active galaxies: ISM galaxies: star formation infrared: galaxies ISM: molecules submillimeter: galaxies
ISSN号	0067-0049
DOI	10.3847/1538-4365/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
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/36013]
专题	中国科学院国家天文台
作者单位	1.Department of Physics, University of Crete, GR-71003 Heraklion, Greece 2.IAASARS, National Observatory of Athens, GR-15236, Penteli, Greece 3.Yunnan Observatories, CAS, Kunming 650011, China 4.National Astronomical Observatories, Chinese Academy of Sciences (CAS), Beijing 100012, China; nanyao.lu@gmail.com 5.South American Center for Astronomy, CAS, Camino El Observatorio 1515, Las Condes, Santiago, Chile 6.Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA 7.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650011, China 8.Purple Mountain Observatory, CAS, Nanjing 210008, China 9.Nucleo de Astronomia de la Facultad de Ingenieria, Universidad Diego Portales, Av. Ejercito Libertador 441, Santiago, Chile 10.Spitzer Science Center, California Institute of Technology, MS 220-6, Pasadena, CA 91125, USA
推荐引用方式 GB/T 7714	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).