Zobrazeno 1 - 10
of 14
pro vyhledávání: '"M. V. Kazandjian"'
Autor:
M. V. Kazandjian, Carla Maria Coppola
Publikováno v:
Rendiconti Lincei. Scienze Fisiche e Naturali. 30:707-714
FRIGUS is a user-friendly Python package for computing cooling functions that depend on gas density, radiation and gas temperatures. The input data are organized as matrices and the computation of the equilibrium level population, as well as the time
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a5f183084560c8d0f7e674f6c363480
https://doi.org/10.1007/s12210-019-00849-x
https://doi.org/10.1007/s12210-019-00849-x
Publikováno v:
Journal of Physical Chemistry A
Journal of Physical Chemistry A, American Chemical Society, 2018, 122 (42), pp.8390-8396. ⟨10.1021/acs.jpca.8b08618⟩
Journal of Physical Chemistry A, American Chemical Society, 2018, 122 (42), pp.8390-8396. ⟨10.1021/acs.jpca.8b08618⟩
The HD molecules are key species for the cooling of pristine gas at temperatures below 100 K. They are also known to be key tracers of H2 in protoplanetary disks and thus, they can be used as a measure of protoplanetary disks mass. Accurate modeling
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3548c1e14118b8b709b3cb9b53ac1a98
https://doi.org/10.1021/acs.jpca.8b08618
https://doi.org/10.1021/acs.jpca.8b08618
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470 (4), pp.4163-4167. ⟨10.1093/mnras/stx1397⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 470 (4), pp.4163-4167. 〈10.1093/mnras/stx1397〉
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 470, 4163-4167
Mon.Not.Roy.Astron.Soc., 2017, 470 (4), pp.4163-4167. ⟨10.1093/mnras/stx1397⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470 (4), pp.4163-4167. ⟨10.1093/mnras/stx1397⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 470 (4), pp.4163-4167. 〈10.1093/mnras/stx1397〉
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 470, 4163-4167
Mon.Not.Roy.Astron.Soc., 2017, 470 (4), pp.4163-4167. ⟨10.1093/mnras/stx1397⟩
Non-thermal photons deriving from radiative transitions among the internal ladder of atoms and molecules are an important source of photons in addition to thermal and stellar sources in many astrophysical environments. In the present work the calcula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ec173f30efac8a19878a46f8f3b1a36
https://doi.org/10.1093/mnras/stx1397
https://doi.org/10.1093/mnras/stx1397
Publikováno v:
Monthly notices of the Royal Astronomical Society (Online) 486 (2019): 1590–1593. doi:10.1093/mnras/stz927
info:cnr-pdr/source/autori:Coppola Carla Maria; Lique François; Mazzia Francesca; Esposito Fabrizio; Kazandjian Mher V./titolo:Temperature and density dependent cooling function for H2 with updated H2%2FH collisional rates/doi:10.1093%2Fmnras%2Fstz927/rivista:Monthly notices of the Royal Astronomical Society (Online)/anno:2019/pagina_da:1590/pagina_a:1593/intervallo_pagine:1590–1593/volume:486
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, 486 (2), pp.1590-1593. ⟨10.1093/mnras/stz927⟩
Monthly Notices of the RAS (0035-8711), 486(2), 1590-1593
info:cnr-pdr/source/autori:Coppola Carla Maria; Lique François; Mazzia Francesca; Esposito Fabrizio; Kazandjian Mher V./titolo:Temperature and density dependent cooling function for H2 with updated H2%2FH collisional rates/doi:10.1093%2Fmnras%2Fstz927/rivista:Monthly notices of the Royal Astronomical Society (Online)/anno:2019/pagina_da:1590/pagina_a:1593/intervallo_pagine:1590–1593/volume:486
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, 486 (2), pp.1590-1593. ⟨10.1093/mnras/stz927⟩
Monthly Notices of the RAS (0035-8711), 486(2), 1590-1593
The energy transfer among the components in a gas determines its fate. Especially at low temperatures, inelastic collisions drive the cooling and the heating mechanisms. In the early Universe as well as in zero- or low- metallicity environments the m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e23f11e757136041f5d0e03b0f62b868
http://arxiv.org/abs/1907.01566
http://arxiv.org/abs/1907.01566
Publikováno v:
Physical Review Letters, 123(2), 021103
The centers of most galaxies contain massive black holes surrounded by dense star clusters. The structure of these clusters determines the rate and properties of observable transient events, such as flares from tidally disrupted stars and gravitation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88e9ad468ffdfe9ad06797d1bcf1f79b
https://pubmed.ncbi.nlm.nih.gov/31386515
https://pubmed.ncbi.nlm.nih.gov/31386515
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 476(3), 4104-4122
We present idealized models of a razor-thin, axisymmetric, Keplerian stellar disc around a massive black hole, and study non-axisymmetric secular instabilities in the absence of either counter-rotation or loss cones. These discs are prograde mono-ene
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::915519399651f752514ab3e45baafb46
http://arxiv.org/abs/1710.11340
http://arxiv.org/abs/1710.11340
Autor:
Savino Longo, Nazzareno Re, Pietro Di Profio, Carla Maria Coppola, Alessandro Marrone, M. V. Kazandjian, José Longo, Cecilia Coletti, Victor Fernandez-Villace, Ionut Tranca, Loriano Storchi, Antonello Pellecchia, Silvia V. Gaastra-Nedea, Iogann Tolbatov
Publikováno v:
Rendiconti Lincei. Scienze Fisische e Naturali, 30(2). Springer
Hydrogen economy has been suggested as a possible green alternative to produce energy, also in the framework of transport applications. According to the specific transport means, different kinds of materials can be adopted. The choice of the most sui
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f8f70a3be851da753953bb7650bf52b
https://research.tue.nl/en/publications/4dc5bb8f-2b53-4b07-a2dd-49f5386e19aa
https://research.tue.nl/en/publications/4dc5bb8f-2b53-4b07-a2dd-49f5386e19aa
Publikováno v:
Astronomy & Astrophysics, 595, A125
Astronomy & Astrophysics
Astronomy and astrophysics, 595(November 2016):A125. EDP Sciences
Astronomy & Astrophysics
Astronomy and astrophysics, 595(November 2016):A125. EDP Sciences
We apply photo-dissociation region (PDR) molecular line emission models, that have varying degrees of enhanced mechanical heating rates, to the gaseous component of simulations of star-forming galaxies taken from the literature. Snapshots of these si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::474cfc29e787147df9ca1eec8a684f1c
http://www.aanda.org/articles/aa/pdf/2016/11/aa23634-14.pdf
http://www.aanda.org/articles/aa/pdf/2016/11/aa23634-14.pdf
Autor:
I. Pelupessy, Frank P. Israel, Marco Spaans, M. J. F. Rosenberg, Carla Maria Coppola, Rowin Meijerink, M. V. Kazandjian
Publikováno v:
Astronomy and astrophysics, 595:A124. EDP Sciences
Astronomy & Astrophysics
Astronomy & Astrophysics, 595, A124
Astronomy & Astrophysics
Astronomy & Astrophysics, 595, A124
Far-infrared molecular emission is an important tool used to understand the excitation mechanisms of the gas in the inter-stellar medium of star-forming galaxies. In the present work, we model the emission from rotational transitions with critical de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9eea30464184ba86ca5e6d7af6c3c9b9
http://arxiv.org/abs/1609.02567
http://arxiv.org/abs/1609.02567
Autor:
A. Weiß, Rolf Güsten, M. A. Requena-Torres, M. J. F. Rosenberg, P. van der Werf, Frank P. Israel, Rowin Meijerink, M. V. Kazandjian
Publikováno v:
Astronomy and astrophysics, 564:A126. EDP Sciences
Starburst galaxies are galaxies or regions of galaxies undergoing intense periods of star formation. Understanding the heating and cooling mechanisms in these galaxies can give us insight to the driving mechanisms that fuel the starburst. Molecular e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2f252b743901beb3ce7cb63826792b2
https://hdl.handle.net/11370/55139af2-be47-400a-b322-b6ccb26561e5
https://hdl.handle.net/11370/55139af2-be47-400a-b322-b6ccb26561e5