Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Jean-Louis Lemaire"'
Autor:
James R. Lyons, M. Eidelsberg, Steven Federman, Nelson de Oliveira, Wim Ubachs, Jean Louis Lemaire, Lisseth Gavilan, Glenn Stark, A. N. Heays
Publikováno v:
Proceedings of the 73rd International Symposium on Molecular Spectroscopy.
Autor:
Mario Accolla, Jean-Louis Lemaire, François Dulieu, E. Congiu, V. Pirronello, H. Chaabouni, G. Manicò
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2013, 429 (4), pp.3200-3206. ⟨10.1093/mnras/sts578⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 429 (4), pp.3200-3206. ⟨10.1093/mnras/sts578⟩
Monthly Notices of the Royal Astronomical Society, 2013, 429 (4), pp.3200-3206. ⟨10.1093/mnras/sts578⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 429 (4), pp.3200-3206. ⟨10.1093/mnras/sts578⟩
We report on an experimental study on the formation of water, through the D + O2 pathway, on a sample of amorphous solid water, i.e. a realistic analogue of the surface of the interstellar grains of dense clouds. For improving our experimental condit
Autor:
S. Aleiferis, J. Bentounes, Lisseth Gavilan, Ana Lacoste, Alexandre Bes, Stephane Bechu, Panagiotis Svarnas, Jean-Louis Lemaire
Publikováno v:
AIP Conference Proceedings
5th International Symposium on Negative Ions, Beams and Sources (NIBS’16)
5th International Symposium on Negative Ions, Beams and Sources (NIBS’16), Sep 2016, Oxford, United Kingdom. pp.020011, ⟨10.1063/1.4995717⟩
5th International Symposium on Negative Ions, Beams and Sources (NIBS’16), Sep 2016, Oxford, United Kingdom. AIP Conference Proceedings, 1869, pp.020011 2017, ⟨10.1063/1.4995717⟩
5th International Symposium on Negative Ions, Beams and Sources (NIBS’16)
5th International Symposium on Negative Ions, Beams and Sources (NIBS’16), Sep 2016, Oxford, United Kingdom. pp.020011, ⟨10.1063/1.4995717⟩
5th International Symposium on Negative Ions, Beams and Sources (NIBS’16), Sep 2016, Oxford, United Kingdom. AIP Conference Proceedings, 1869, pp.020011 2017, ⟨10.1063/1.4995717⟩
International audience; Volume production of H- negative ions is mostly attributed to the dissociative attachment (DA) of electrons to ro-vibrationally excited molecules.1,2 Apart from the main formation path for enriching the plasma with these molec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35f36c13d2b2c85ceedd4f02b993748a
https://hal-insu.archives-ouvertes.fr/insu-01616032
https://hal-insu.archives-ouvertes.fr/insu-01616032
Autor:
T Sabri, Damien Salomon, E. Foy, Cornelia Jäger, Lisseth Gavilan, Jean-Louis Lemaire, Alexandre Simionovici, Th. Henning, S. Yagoubi, Gema Martínez-Criado
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 587, pp.A144. ⟨10.1051/0004-6361/201527708⟩
Astronomy and Astrophysics-A&A, 2016, 587, pp.A144. ⟨10.1051/0004-6361/201527708⟩
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 587, pp.A144. ⟨10.1051/0004-6361/201527708⟩
Astronomy and Astrophysics-A&A, 2016, 587, pp.A144. ⟨10.1051/0004-6361/201527708⟩
[Context] Protoplanetary disks, interstellar clouds, and active galactic nuclei contain X-ray-dominated regions. X-rays interact with the dust and gas present in such environments. While a few laboratory X-ray irradiation experiments have been perfor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb533a32bea261875a0e54e7d203e45f
http://hdl.handle.net/10261/185984
http://hdl.handle.net/10261/185984
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 424:2961-2970
The formation of H2 in the interstellar medium (ISM) involves complex processes, some of which are still not understood. In cold regions, it is assumed that H2 formation follows Langmuir kinetics, i.e. the immediate desorption of incoming atoms or mo
Autor:
Julien Pilmé, M. Lattelais, X. Michaut, François Dulieu, Jean-Louis Lemaire, H. Mokrane, Pascal Jeseck, C. Romanzin, E. Congiu, H. Chaabouni, Jean-Hugues Fillion, S. Baouche, F. Pauzat, Mathieu Bertin, C. Minot, Y. Ellinger
Publikováno v:
EAS Publications Series. 58:349-352
Context. Over 20 of the ~150 different species detected in the interstellar and circumstellar media have also been identified in icy environments. For most of the species observed so far in the interstellar medium (ISM), the most abundant isomer of a
Autor:
X. Michaut, H. Mokrane, Jean-Louis Lemaire, J. H. Fillion, François Dulieu, H. Chaabouni, E. Congiu, M. Chehrouri, E. Matar
Publikováno v:
Phys. Chem. Chem. Phys.. 13:2172-2178
Nuclear spin conversion (NSC) of ortho- to para-H(2) and para- to ortho-D(2) has been investigated on an amorphous solid water (ASW) surface at 10 K, in the presence of co-adsorbed O(2). The dynamics of the nuclear spin conversion could be revealed b
Autor:
M. Gustafsson, S. Diana, G. Pineau des Forêts, David J. Field, T. Ravkilde, L. E. Kristensen, Jean-Louis Lemaire, S. Cabrit
Publikováno v:
Kristensen, L E, Ravkilde, T L, Des Forêts, G P, Cabrit, S, Field, D, Gustafsson, M, Diana, S & Lemaire, J L 2008, ' Observational 2D model of H 2 emission from a bow shock in the Orion Molecular Cloud ', Astronomy and Astrophysics, vol. 477, no. 1, pp. 203-211 . https://doi.org/10.1051/0004-6361:20078100
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2008, 477, pp.203-211. ⟨10.1051/0004-6361:20078100⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2008, 477, pp.203-211. ⟨10.1051/0004-6361:20078100⟩
International audience; Aims:We present a new method for reproducing high spatial resolution observations of bow shocks by using 1D plane parallel shock models. As an example we analyse one bow shock located in the Orion Molecular Cloud (OMC1). Metho
Publikováno v:
Physical Chemistry Chemical Physics
Physical Chemistry Chemical Physics, Royal Society of Chemistry, 2015, 17 (44), pp.30148-30157. ⟨10.1039/C5CP03985A⟩
Physical Chemistry Chemical Physics, 2015, 17 (44), pp.30148-30157. ⟨10.1039/C5CP03985A⟩
Physical Chemistry Chemical Physics, Royal Society of Chemistry, 2015, 17 (44), pp.30148-30157. ⟨10.1039/C5CP03985A⟩
Physical Chemistry Chemical Physics, 2015, 17 (44), pp.30148-30157. ⟨10.1039/C5CP03985A⟩
We study the adsorption and desorption of three isotopologues of molecular hydrogen mixed on 10 ML of porous amorphous water ice (ASW) deposited at 10 K. Thermally programmed desorption (TPD) of H2, D2 and HD adsorbed at 10 K have been performed with
Autor:
M. Eidelsberg, N. de Oliveira, Laurent Nahon, Jean-Louis Lemaire, James R. Lyons, Alan N. Heays, S. R. Federman, Glenn Stark
Publikováno v:
Proceedings of the International Astronomical Union. 11
The photochemistry of CO and its isotoplogues affects the structure and evolution of many astronomical environments, including interstellar clouds, circumstellar disks around newly formed stars, and the envelopes surrounding highly evolved stars. Whe