Zobrazeno 1 - 10
of 249
pro vyhledávání: '"T. Montmerle"'
Publikováno v:
Atmospheric Measurement Techniques, Vol 13, Pp 2279-2298 (2020)
This paper presents the potential of nonlinear and linear versions of an observation operator for simulating polarimetric variables observed by weather radars. These variables, deduced from the horizontally and vertically polarized backscattered radi
Externí odkaz:
https://doaj.org/article/8323fe4a99e744a18cdfd11d693e23fd
Publikováno v:
Nonlinear Processes in Geophysics, Vol 23, Iss 1, Pp 1-12 (2016)
In numerical weather prediction, the problem of estimating initial conditions with a variational approach is usually based on a Bayesian framework associated with a Gaussianity assumption of the probability density functions of both observations and
Externí odkaz:
https://doaj.org/article/5709928e9ac04e5ab9996a70e4b9a182
Autor:
Vera Jatenco-Pereira, H. D. Perottoni, T. Montmerle, M. Borges Fernandes, F. Navarete, Phillip A. B. Galli, Antonio Kanaan, William Schoenell, T. Ribeiro, Beatriz Luci Fernandes, T. Santos-Silva, Jane Gregorio-Hetem, A. Hetem
An exotic environment surrounds the young stellar groups associated with the Canis Major (CMa) OB1/R1 region, which probably was formed under feedback from at least three supernova events having occurred a few million years ago. We use astrometric da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::242eea78879aea22bbb65994cba85b22
Autor:
Edgar Mendoza, Bertrand Lefloch, Beatriz L. Fernandes, Jane Gregorio-Hetem, T. Montmerle, A. Hetem, M. De Simone
Publikováno v:
Astronomy & Astrophysics. 654:A150
The relationship between young stellar clusters and respective parental molecular clouds is still an open issue: for instance, are the similarities between substructures of clouds and clusters just a coincidence? Or would they be the indication of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f02167d2f177924bf4ba494c319f985
https://doi.org/10.1051/0004-6361/202141535
https://doi.org/10.1051/0004-6361/202141535
Autor:
Ph. André, A. Hughes, V. Guillet, F. Boulanger, A. Bracco, E. Ntormousi, D. Arzoumanian, A.J. Maury, J.-Ph. Bernard, S. Bontemps, I. Ristorcelli, J.M. Girart, F. Motte, K. Tassis, E. Pantin, T. Montmerle, D. Johnstone, S. Gabici, A. Efstathiou, S. Basu, M. Béthermin, H. Beuther, J. Braine, J. Di Francesco, E. Falgarone, K. Ferrière, A. Fletcher, M. Galametz, M. Giard, P. Hennebelle, A. Jones, A
Publikováno v:
Publications of the Astronomical Society of Australia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r3c4b2081b22::bd68e7e5ac33e38cc5551838c1528f99
Akademický článek
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Autor:
Leisa K. Townsley, T. Montmerle
Publikováno v:
Astronomische Nachrichten. 333:355-360
As a result of feedback from massive stars, via their intense winds and/or supernova explosions, massive star-forming regions are entirely filled with hot, X-ray emitting plasmas, which escape into the ambient ISM. As shown recently by Townsley et al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9060488f354eb1d6cfa34a07b65d3368
https://doi.org/10.1002/asna.201211678
https://doi.org/10.1002/asna.201211678
The close classical T Tauri binary V4046 Sgr: complex magnetic fields and distributed mass accretion
Autor:
Manuel Güdel, D. P. Huenemoerder, A. Maggio, Gregg A. Wade, J.-F. Donati, G. G. Sacco, Costanza Argiroffi, Francesco Damiani, Jerome Bouvier, G. A. J. Hussain, T. Montmerle, Scott G. Gregory, Joel H. Kastner, Marc Audard, S. H. P. Alencar
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 417:1747-1759
We report here the first results of a multi-wavelength campaign focussing on magnetospheric accretion processes within the close binary system V4046 Sgr, hosting two partly-convective classical T Tauri stars of masses ~0.9 Msun and age ~12 Myr. In th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cea3655b8e5a9f9088aa3ead08a6aadf
https://doi.org/10.1111/j.1365-2966.2011.19366.x
https://doi.org/10.1111/j.1365-2966.2011.19366.x
Autor:
T. Montmerle
Publikováno v:
EAS Publications Series. 51:299-310
We briefly review the feedback effects of massive stars, via their stellar winds and supernova explosions, on the star-forming regions in which they were born. We give a few examples, spanning a wide range of spatial scales, from ∼100 pc out to ∼
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::41e0b1ba81377fcaa2e25d53eb9fb6e5
https://doi.org/10.1051/eas/1151015
https://doi.org/10.1051/eas/1151015
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, 2008, 387, pp.L23. ⟨10.1111/j.1745-3933.2008.00474.x⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2008, 387, pp.L23. ⟨10.1111/j.1745-3933.2008.00474.x⟩
The origin of the magnetic fields in neutron stars, and the physical differences between magnetars and strongly magnetised radio pulsars are still under vigorous debate. It has been suggested that the properties of the progenitors of neutron stars (t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e9bf7dc071ddba6707b0f5e8a713673
https://doi.org/10.1111/j.1745-3933.2008.00474.x
https://doi.org/10.1111/j.1745-3933.2008.00474.x