WFRF:(Genzel R.)
Sökning: WFRF:(Genzel R.) > (2020-2021) > Molecular outflows ...
LIBRIS Formathandbok (Information om MARC21)
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06810naa a2200625 4500 | |
| 001 | oai:research.chalmers.se:8cc5e527-e8f3-4c9a-85d6-a075989540de | |
| 003 | SwePub | |
| 008 | 200131s2020 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2019368032 DOI |
| 024 | 7 | a https://research.chalmers.se/publication/5188222 URI |
| 024 | 7 | a https://research.chalmers.se/publication/5151792 URI |
| 040 | a (SwePub)cth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a art2 swepub-publicationtype |
| 072 | 7 | a ref2 swepub-contenttype |
| 100 | 1 | a Lutz, D.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 245 | 1 0 | a Molecular outflows in local galaxies: Method comparison and a role of intermittent AGN driving |
| 264 | c 2020-01-22 | |
| 264 | 1 | b EDP Sciences,c 2020 |
| 338 | a electronic2 rdacarrier | |
| 520 | a We report new detections and limits from a NOEMA and ALMA CO(1-0) search for molecular outflows in 13 local galaxies with high far-infrared surface brightness, and combine these with local universe CO outflow results from the literature. The CO line ratios and spatial outflow structure of our targets provide some constraints on the conversion steps from observables to physical quantities such as molecular mass outflow rates. Where available, ratios between outflow emission in higher J CO transitions and in CO(1-0) are typically consistent with excitation R-i1 less than or similar to 1. However, for IRAS 13120 5453, R-31 = 2.10 +/- 0.29 indicates optically thin CO in the outflow. Like much of the outflow literature, we use ff CO(1 0) = 0.8, and we present arguments for using C = 1 in deriving molecular mass outflow rates. (M)over dot(out) = CM(out)v(out)/R-out. We compare the two main methods for molecular outflow detection: CO millimeter interferometry and Herschel OH-based spectroscopic outflow searches. For 26 sources studied with both methods, we find an 80% agreement in detecting vout & 150 km s 1 outflows, and non-matches can be plausibly ascribed to outflow geometry and signal-to-noise ratio. For a published sample of 12 bright ultraluminous infrared galaxies with detailed OH-based outflow modeling, CO outflows are detected in all but one. Outflow masses, velocities, and sizes for these 11 sources agree well between the two methods, and modest remaining di fferences may relate to the di fferent but overlapping regions sampled by CO emission and OH absorption. Outflow properties correlate better with active galactic nucleus (AGN) luminosity and with bolometric luminosity than with far-infrared surface brightness. The most massive outflows are found for systems with current AGN activity, but significant outflows in nonAGN systems must relate to star formation or to AGN activity in the recent past. We report scaling relations for the increase of outflow mass, rate, momentum rate, and kinetic power with bolometric luminosity. Short flow times of similar to 10(6) yr and some sources with resolved multiple outflow episodes support a role of intermittent driving, likely by AGNs. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a galaxies: active | |
| 653 | a galaxies: kinematics and dynamics | |
| 653 | a galaxies: ISM | |
| 700 | 1 | a Sturm, E.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Janssen, A.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Veilleux, S.u Space Telescope Science Institute (STScI),University Of Cambridge,University of Maryland4 aut |
| 700 | 1 | a Aalto, Susanne,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)saalto |
| 700 | 1 | a Cicone, C.u Istituto nazionale di astrofisica (INAF),Universitetet i Oslo,University of Oslo4 aut |
| 700 | 1 | a Contursi, A.u Institut de Radioastronomie Millimétrique (IRAM),Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Davies, R. I.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Feruglio, C.u Istituto nazionale di astrofisica (INAF)4 aut |
| 700 | 1 | a Fischer, J.u George Mason University4 aut |
| 700 | 1 | a Fluetsch, A.u University Of Cambridge4 aut |
| 700 | 1 | a Garcia-Burillo, S.u Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)4 aut |
| 700 | 1 | a Genzel, R.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Gonzalez-Alfonso, E.u Universidad de Alcala,University of Alcalá4 aut |
| 700 | 1 | a Gracia-Carpio, J.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Herrera-Camus, R.u Universidad de Concepción,University of Concepcion,Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Maiolino, R.u University Of Cambridge4 aut |
| 700 | 1 | a Schruba, A.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Shimizu, T.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Sternberg, A.u Tel Aviv University4 aut |
| 700 | 1 | a Tacconi, L. J.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 700 | 1 | a Weiss, A.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
| 710 | 2 | a Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG)b Space Telescope Science Institute (STScI)4 org |
| 773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 633q 633x 0004-6361x 1432-0746 |
| 856 | 4 | u https://research.chalmers.se/publication/518822/file/518822_Fulltext.pdfx primaryx freey FULLTEXT |
| 856 | 4 | u https://www.aanda.org/articles/aa/pdf/2020/01/aa36803-19.pdf |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/201936803 |
| 856 | 4 8 | u https://research.chalmers.se/publication/518822 |
| 856 | 4 8 | u https://research.chalmers.se/publication/515179 |
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