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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004319naa a2200541 4500
001oai:research.chalmers.se:6355c223-8605-4e1a-992a-34f5befca410
003SwePub
008171007s2016 | |||||||||||000 ||eng|
024a https://research.chalmers.se/publication/2464882 URI
024a https://doi.org/10.1051/0004-6361/2016290732 DOI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Muller, Sebastien,d 1976u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)mullers
2451 0a OH+ and H2O+ absorption toward PKS 1830-211
264 c 2016-11-16
264 1b 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 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a 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
700a Müller, H. S. P.u Universität zu Köln,University of Cologne4 aut
700a Black, John H,d 1949u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)jblack
700a Beelen, A.u Institut d'Astrophysique Spatiale4 aut
700a Combes, F.u Centre national de la recherche scientifique (CNRS)4 aut
700a Curran, S.J.u Victoria University of Wellington4 aut
700a Gerin, M.u Ecole Normale Superieure (ENS)4 aut
700a Guélin, M.u Ecole Normale Superieure (ENS),Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a 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
700a Martín, S.u European Southern Observatory Santiago4 aut
700a Aalto, Susanne,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)saalto
700a Falgarone, E.u Ecole Normale Superieure (ENS)4 aut
700a 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
700a Schilke, P.u Universität zu Köln,University of Cologne4 aut
700a Wiklind, Tommy,d 1957u Catholic University of America4 aut0 (Swepub:cth)wiklind
700a Zwaan, M. A.u European Southern Observatory (ESO)4 aut
710a Chalmers tekniska högskolab Universität zu Köln4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 595, s. A128(1-10)q 595<A128(1-10)x 0004-6361x 1432-0746
856u http://publications.lib.chalmers.se/records/fulltext/246488/local_246488.pdfx primaryx freey FULLTEXT
856u https://www.aanda.org/articles/aa/pdf/2016/11/aa29073-16.pdf
8564 8u https://research.chalmers.se/publication/246488
8564 8u https://doi.org/10.1051/0004-6361/201629073

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