The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder - V. Rotational measurements of NGC 891
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作者:
Benson, Chris S.
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Univ Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, CanadaUniv Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
Benson, Chris S.
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Spencer, L. D.
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Univ Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, CanadaUniv Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
Spencer, L. D.
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Valtchanov, I
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European Space Astron Ctr, Operat Dept, Telespazio Vega UK ESA, E-28691 Villanueva De La Canada, SpainUniv Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
Valtchanov, I
[2
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Scott, J.
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Univ Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, CanadaUniv Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
Scott, J.
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Hladczuk, N.
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European Space Astron Ctr, ESA, Camino Bajo Castillo, E-28692 Madrid, Spain
Gran TeCan SA, Inst Astrofis Canarias, C Via Lactea S-N, E-38205 San Cristobal De Laguna, Sc De Tenerife, SpainUniv Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
Hladczuk, N.
[3
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机构:
[1] Univ Lethbridge, Inst Space Imaging Sci, Departmentof Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
[2] European Space Astron Ctr, Operat Dept, Telespazio Vega UK ESA, E-28691 Villanueva De La Canada, Spain
[3] European Space Astron Ctr, ESA, Camino Bajo Castillo, E-28692 Madrid, Spain
[4] Gran TeCan SA, Inst Astrofis Canarias, C Via Lactea S-N, E-38205 San Cristobal De Laguna, Sc De Tenerife, Spain
The ESA Herschel Spectral and Photometric Imaging Receiver (SPIRE) Fourier Transform Spectrometer (FTS) Spectral Feature Finder (FF) project is an automated spectral feature fitting routine developed within the SPIRE instrument team to extract all prominent spectral features from all publicly available SPIRE FTS observations. In this work, we demonstrate the use of the FF information extracted from three observations of the edge-on spiral galaxy NGC 891 to measure the rotation of NII and CI gas at far-infrared frequencies in complement to radio observations of the [HI] 21-cm line and the CO(1-0) transition as well as optical measurements of H alpha. We find that measurements of both NII and CI gas follow a similar velocity profile to that of HI and H alpha showing a correlation between neutral and ionized regions of the interstellar medium in the disc of NGC 891.