Estimation of physical conditions in the cold phase of the interstellar medium in the sub-DLA system at z = 2.06 in the spectrum of the quasar J 2123

Estimation of physical conditions in the cold phase of the interstellar medium in the sub-DLA system at z = 2.06 in the spectrum of the quasar J 2123–0050

Published:2016-03 Issue:3 Volume:42 Page:137-162
ISSN:1063-7737
Container-title:Astronomy Letters
language:en
Short-container-title:Astron. Lett.

Author:

Klimenko V. V.,Balashev S. A.,Ivanchik A. V.,Varshalovich D. A.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S1063773716030038.pdf

Reference80 articles.

1. T. Abel, P. Anninos, Y. Zhang, and M. L. Norman, New Astron. 2, 181 (1997).

2. H. Abgrall and E. Roueff, Astron. Astrophys. 445, 361 (2006).

3. H. Abgrall, J. Le Bourlot, G. Pineau des Forets, E. Roueff, D. R. Flower, and L. Heck, Astron. Astrophys. 253, 525 (1992).

4. E. Abrahamsson, R. V. Krems, and A. Dalgarno, Astrophys. J. 654, 1172 (2007).

5. P. A. R. Ade, N. Aghanim, M. Arnaud, M. Ashdown, J. Aumont, C. Baccigalupi, A. J. Banday, R. B. Barreiro, et al., arXiv: 1502. 01589 (2015).

Cited by 12 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Excitation of CO molecules in diffuse gas over cosmic history;Monthly Notices of the Royal Astronomical Society;2024-08-07

2. Neutral carbon in diffuse interstellar medium: abundance matching with H2 for damped Lyman alpha systems at high redshifts;Monthly Notices of the Royal Astronomical Society;2023-12-23

3. HD molecules at high redshift: cosmic ray ionization rate in the diffuse interstellar medium;Monthly Notices of the Royal Astronomical Society;2021-05-27

4. Physical conditions in the diffuse interstellar medium of local and high-redshift galaxies: measurements based on the excitation of H2 rotational and C i fine-structure levels;Monthly Notices of the Royal Astronomical Society;2020-09-16

5. Influence of Radiative Pumping on the HD Rotational Level Populations in Diffuse Molecular Clouds of the Interstellar Medium;Astronomy Letters;2020-04