Hydrogen Fluoride toward Luminous Nearby Galaxies: NGC 253 and NGC 4945
arXiv:1402.6619 · doi:10.1088/0004-637X/785/1/22
Abstract
We present the detection of hydrogen fluoride, HF, in two luminous nearby galaxies NGC 253 and NGC 4945 using the Heterodyne Instrument for the Far-Infrared (HIFI) on board the Herschel Space Observatory. The HF line toward NGC 253 has a P-Cygni profile, while an asymmetric absorption profile is seen toward NGC 4945. The P-Cygni profile in NGC 253 suggests an outflow of molecular gas with a mass of M(H) 1 10 M and an outflow rate as large as M 6.4 M yr. In the case of NGC 4945, the axisymmetric velocity components in the HF line profile is compatible with the interpretation of a fast-rotating nuclear ring surrounding the nucleus and the presence of inflowing gas. The gas falls into the nucleus with an inflow rate of 1.2 M yr, inside a inner radius of 200 pc. The gas accretion rate to the central AGN is much smaller, suggesting that the inflow can be triggering a nuclear starburst. From these results, the HF line is seen to provide an important probe of the kinematics of absorbing material along the sight-line to nearby galaxies with bright dust continuum and a promising new tracer of molecular gas in high-redshift galaxies.
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Cited by in corpus (15)
- A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns
- HIFI Spectroscopy of submm Lines in Nuclei of Actively Star Forming Galaxies
- Molecular line emission in NGC 4945, imaged with ALMA
- A Herschel/HIFI Legacy Survey of HF and H2O in the Galaxy: Probing Diffuse Molecular Cloud Chemistry
- A thorough view of the nuclear region of NGC 253 - Combined Herschel, SOFIA and APEX dataset
- The ionization rates of galactic nuclei and disks from Herschel/HIFI observations of water and its associated ions
- ExoMol photodissociation cross sections I: HCl and HF
- Detection of 36 GHz Class I Methanol Maser Emission Towards NGC 4945
- The ramp-up of interstellar medium enrichment at z>4
- Collisional quenching of highly rotationally excited HF
- Origin of hydrogen fluoride emission in the Orion Bar: An excellent tracer for CO-dark H2 gas clouds
- Uncovering the nucleus candidate for NGC 253
- Three-dimensional distribution of hydrogen fluoride gas toward NGC6334 I and I(N)
- Etching glass in the early Universe: Luminous HF and water emission in a QSO-SMG pair at z=4.7
- ArH+ and H2O+ absorption towards luminous galaxies