Search: WFRF:(Muller Susanne) > OH+ and H2O+ absorp...
Fältnamn | Indikatorer | Metadata |
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000 | 04319naa a2200541 4500 | |
001 | oai:research.chalmers.se:6355c223-8605-4e1a-992a-34f5befca410 | |
003 | SwePub | |
008 | 171007s2016 | |||||||||||000 ||eng| | |
024 | 7 | a https://research.chalmers.se/publication/2464882 URI |
024 | 7 | a https://doi.org/10.1051/0004-6361/2016290732 DOI |
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 Muller, Sebastien,d 1976u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)mullers |
245 | 1 0 | a OH+ and H2O+ absorption toward PKS 1830-211 |
264 | c 2016-11-16 | |
264 | 1 | b EDP Sciences,c 2016 |
338 | a electronic2 rdacarrier | |
520 | a We report the detection of OH+ and H2O+ in the z = 0.89 absorber toward the lensed quasar PKS 1830-211. The abundance ratio of OH+ and H2O+ is used to quantify the molecular hydrogen fraction (fH2) and the cosmic-ray ionization rate of atomic hydrogen (ζH) along two lines of sight, located at 2 kpc and 4 kpc to either side of the absorber's center. The molecular fraction decreases outward, from 0.04 to 0.02, comparable to values measured in the Milky Way at similar galactocentric radii. For ζH , we find values of 2 × 10-14 s-1 and 3 × 10-15 s-1, respectively, which are slightly higher than in the Milky Way at comparable galactocentric radii, possibly due to a higher average star formation activity in the z = 0.89 absorber. The ALMA observations of OH+, H2O+, and other hydrides toward PKS 1830-211reveal the multi-phase composition of the absorbing gas. Taking the column density ratios along the southwest and northeast lines of sight as a proxy of molecular fraction, we classify the species ArH+, OH+, H2Cl+, H2O+, CH, and HF as tracing gases increasingly more molecular. Incidentally, our data allow us to improve the accuracy of H2O+ rest frequencies and thus refine the spectroscopic parameters. | |
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 quasar absorption lines | |
653 | a quasars | |
653 | a interstellar molecules | |
653 | a galaxies: abundances | |
700 | 1 | a Müller, H. S. P.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Black, John H,d 1949u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)jblack |
700 | 1 | a Beelen, A.u Institut d'Astrophysique Spatiale4 aut |
700 | 1 | a Combes, F.u Centre national de la recherche scientifique (CNRS)4 aut |
700 | 1 | a Curran, S.J.u Victoria University of Wellington4 aut |
700 | 1 | a Gerin, M.u Ecole Normale Superieure (ENS)4 aut |
700 | 1 | a Guélin, M.u Ecole Normale Superieure (ENS),Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Henkel, C.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG),King Abdulaziz University4 aut |
700 | 1 | a Martín, S.u European Southern Observatory Santiago4 aut |
700 | 1 | a Aalto, Susanne,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)saalto |
700 | 1 | a Falgarone, E.u Ecole Normale Superieure (ENS)4 aut |
700 | 1 | a Menten, K. M.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 Schilke, P.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Wiklind, Tommy,d 1957u Catholic University of America4 aut0 (Swepub:cth)wiklind |
700 | 1 | a Zwaan, M. A.u European Southern Observatory (ESO)4 aut |
710 | 2 | a Chalmers tekniska högskolab Universität zu Köln4 org |
773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 595, s. A128(1-10)q 595<A128(1-10)x 0004-6361x 1432-0746 |
856 | 4 | u http://publications.lib.chalmers.se/records/fulltext/246488/local_246488.pdfx primaryx freey FULLTEXT |
856 | 4 | u https://www.aanda.org/articles/aa/pdf/2016/11/aa29073-16.pdf |
856 | 4 8 | u https://research.chalmers.se/publication/246488 |
856 | 4 8 | u https://doi.org/10.1051/0004-6361/201629073 |
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