Zobrazeno 1 - 4
of 4
pro vyhledávání: '"V. H. M. Phan"'
Autor:
P. Mertsch, V. H. M. Phan
Publikováno v:
Astronomy & Astrophysics. 671:A54
The 21-cm emission from atomic hydrogen (HI) is one of the most important tracers of the structure and dynamics of the interstellar medium. Thanks to Galactic rotation, the line is Doppler shifted and, assuming a model for the velocity field, data fr
Autor:
Regis Terrier, V. H. M. Phan, Julian Krause, Mélissa D. Menu, Stefano Gabici, Giovanni Morlino, Jacco Vink
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy & Astrophysics, 635:A40. EDP Sciences
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy & Astrophysics, 635:A40. EDP Sciences
Astronomy & Astrophysics
Supernova remnants interacting with molecular clouds are ideal laboratories to study the acceleration of particles at shock waves and their transport and interactions in the surrounding interstellar medium. In this paper, we focus on the supernova re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da3ea086579367e90a04c8a03e5c8e0a
https://hal-cea.archives-ouvertes.fr/cea-02499011/file/aa36927-19.pdf
https://hal-cea.archives-ouvertes.fr/cea-02499011/file/aa36927-19.pdf
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 485 (2), pp.2276-2280. ⟨10.1093/mnras/stz555⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 485 (2), pp.2276-2280. ⟨10.1093/mnras/stz555⟩
Monthly Notices of the Royal Astronomical Society, 2019, 485 (2), pp.2276-2280. ⟨10.1093/mnras/stz555⟩
Mon.Not.Roy.Astron.Soc., 2019, 485 (2), pp.2276-2280. ⟨10.1093/mnras/stz555⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 485 (2), pp.2276-2280. ⟨10.1093/mnras/stz555⟩
Monthly Notices of the Royal Astronomical Society, 2019, 485 (2), pp.2276-2280. ⟨10.1093/mnras/stz555⟩
International audience; Low-energy cosmic rays are the major ionization agents of molecular clouds. However, it has been shown that, if the cosmic ray spectrum measured by Voyager 1 is representative of the whole Galaxy, the predicted ionization rate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2edee4fef5fe908199e477bc26bb1807
https://hal.archives-ouvertes.fr/hal-01999994
https://hal.archives-ouvertes.fr/hal-01999994
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 480 (4), pp.5167-5174. ⟨10.1093/mnras/sty2235⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 480 (4), pp.5167-5174. ⟨10.1093/mnras/sty2235⟩
Monthly Notices of the Royal Astronomical Society, 2018, 480 (4), pp.5167-5174. ⟨10.1093/mnras/sty2235⟩
Mon.Not.Roy.Astron.Soc., 2018, 480 (4), pp.5167-5174. ⟨10.1093/mnras/sty2235⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 480 (4), pp.5167-5174. ⟨10.1093/mnras/sty2235⟩
Monthly Notices of the Royal Astronomical Society, 2018, 480 (4), pp.5167-5174. ⟨10.1093/mnras/sty2235⟩
Cosmic rays are usually assumed to be the main ionization agent for the interior of molecular clouds where UV and X-ray photons cannot penetrate. Here we test this hypothesis by limiting ourselves to the case of diffuse clouds and assuming that the a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff04b14deda94a0b87f0f20c8e6eb1cb
https://hal.archives-ouvertes.fr/hal-01791956
https://hal.archives-ouvertes.fr/hal-01791956