How does C+ recombine in diffuse molecular gas?
A&A, 527 (2011) A45
Published online: 2011-01-24
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
Prachi Khatri, Cristiano Porciani, Emilio Romano-Díaz, Daniel Seifried and Alexander SchäbeAstronomy & Astrophysics 688 A194 (2024)
https://doi.org/10.1051/0004-6361/202449640
Excitation of CO molecules in diffuse gas over cosmic history
V V Klimenko, S A Balashev, P Noterdaeme, R Srianand and A V IvanchikMonthly Notices of the Royal Astronomical Society 533 (2) 1367 (2024)
https://doi.org/10.1093/mnras/stae1863
Neutral carbon in diffuse interstellar medium: abundance matching with H2 for damped Lyman alpha systems at high redshifts
S A Balashev and D N KosenkoMonthly Notices of the Royal Astronomical Society 527 (4) 12109 (2023)
https://doi.org/10.1093/mnras/stad3971
Dust, CO, and [C i]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
L Dunne, S J Maddox, P P Papadopoulos, R J Ivison and H L GomezMonthly Notices of the Royal Astronomical Society 517 (1) 962 (2022)
https://doi.org/10.1093/mnras/stac2098
Methanol in the RNA world: An astrochemical perspective
Thomas Mathew, Pierre Mothé Esteves and G. K. Surya PrakashFrontiers in Astronomy and Space Sciences 9 (2022)
https://doi.org/10.3389/fspas.2022.809928
Photodissociation and X-Ray-Dominated Regions
Mark G. Wolfire, Livia Vallini and Mélanie ChevanceAnnual Review of Astronomy and Astrophysics 60 (1) 247 (2022)
https://doi.org/10.1146/annurev-astro-052920-010254
Dust continuum, CO, and [C i] 1 − 0 lines: self-consistent H2 mass estimates and the possibility of globally CO-‘dark’ galaxies at z = 0.35
L Dunne, S J Maddox, C Vlahakis and H L GomezMonthly Notices of the Royal Astronomical Society 501 (2) 2573 (2021)
https://doi.org/10.1093/mnras/staa3526
CO Emission and CO Hot Spots in Diffuse Molecular Gas
Harvey S. LisztThe Astrophysical Journal 897 (1) 104 (2020)
https://doi.org/10.3847/1538-4357/ab9601
A Simple and Accurate Network for Hydrogen and Carbon Chemistry in the Interstellar Medium
Munan Gong, Eve C. Ostriker and Mark G. WolfireThe Astrophysical Journal 843 (1) 38 (2017)
https://doi.org/10.3847/1538-4357/aa7561
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
V. V. Klimenko, S. A. Balashev, A. V. Ivanchik and D. A. VarshalovichAstronomy Letters 42 (3) 137 (2016)
https://doi.org/10.1134/S1063773716030038
THERMAL PRESSURES IN THE INTERSTELLAR MEDIUM OF THE MAGELLANIC CLOUDS*
Daniel E. Welty, James T. Lauroesch, Tony Wong and Donald G. YorkThe Astrophysical Journal 821 (2) 118 (2016)
https://doi.org/10.3847/0004-637X/821/2/118
Non-equilibrium cooling rate for a collisionally cooled metal-enriched gas
Evgenii O. VasilievMonthly Notices of the Royal Astronomical Society 431 (1) 638 (2013)
https://doi.org/10.1093/mnras/stt189
The CO-to-H2 Conversion Factor
Alberto D. Bolatto, Mark Wolfire and Adam K. LeroyAnnual Review of Astronomy and Astrophysics 51 (1) 207 (2013)
https://doi.org/10.1146/annurev-astro-082812-140944
Approximations for modelling CO chemistry in giant molecular clouds: a comparison of approaches
Simon C. O. Glover and Paul C. ClarkMonthly Notices of the Royal Astronomical Society no (2012)
https://doi.org/10.1111/j.1365-2966.2011.20260.x