Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Patrick Guillout"'
Autor:
Patrick Guillout, Tsevi Mazeh, Yveline Lebreton, Jean-Baptiste Le Bouquin, Benoit Famaey, F. Kiefer, Frédéric Arenou, J.-B. Salomon, Henri M. J. Boffin, Jean-Louis Halbwachs, Dimitri Pourbaix
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, 2020, 496 (2), pp.1355-1368. ⟨10.1093/mnras/staa1571⟩
Monthly notices of the Royal Astronomical Society, 496 (2
Monthly Notices of the Royal Astronomical Society, 2020, 496 (2), pp.1355-1368. ⟨10.1093/mnras/staa1571⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 496 (2), pp.1355-1368. ⟨10.1093/mnras/staa1571⟩
Monthly notices of the Royal Astronomical Society, 496 (2
Monthly Notices of the Royal Astronomical Society, 2020, 496 (2), pp.1355-1368. ⟨10.1093/mnras/staa1571⟩
Double-lined spectroscopic binaries (SB2s) are one of the main sources of stellar masses, as additional observations are only needed to give the inclinations of the orbital planes in order to obtain the individual masses of the components. For this r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a76470b04241453771312c659877ed9c
https://hal.archives-ouvertes.fr/hal-02881420/document
https://hal.archives-ouvertes.fr/hal-02881420/document
Autor:
Antonio Frasca, Nicolas Grosso, Patrick Guillout, F. X. Pineau, A. Klutsch, Beate Stelzer, D. Montes
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, ⟨10.1051/0004-6361/201937216⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Astronomy and Astrophysics-A&A, 2020, ⟨10.1051/0004-6361/201937216⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, ⟨10.1051/0004-6361/201937216⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Astronomy and Astrophysics-A&A, 2020, ⟨10.1051/0004-6361/201937216⟩
Young field stars are hardly distinguishable from older ones because their space motion rapidly mixes them with the stellar population of the Galactic plane. Nevertheless, a careful target selection allows for young stars to be spotted throughout the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c35038a91ad657cc73d5ce96f50853e
https://hal.archives-ouvertes.fr/hal-02565954/document
https://hal.archives-ouvertes.fr/hal-02565954/document
Autor:
Patrick Guillout, Caroline Soubiran, Tsevi Mazeh, Flavien Kiefer, Jean-Louis Halbwachs, Yveline Lebreton, Dimitri Pourbaix, Rodrigo A. Ibata, Benoit Famaey, Frédéric Arenou
Publikováno v:
Monthly notices of the Royal Astronomical Society, 474
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2018, 474 (1), pp.731-745. ⟨10.1093/mnras/stx2794⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 474 (1), pp.731-745. ⟨10.1093/mnras/stx2794⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2018, 474 (1), pp.731-745. ⟨10.1093/mnras/stx2794⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 474 (1), pp.731-745. ⟨10.1093/mnras/stx2794⟩
The orbital motion of non-contact double-lined spectroscopic binaries (SB2s), with periods of a few tens of days to several years, holds unique, accurate information on individual stellar masses, which only long-term monitoring can unlock. The combin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c93ac78977441c89c0b936730f76bd3
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/266928
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/266928
Autor:
Filippos Koliopanos, Manfred W. Pakull, I. Traulsen, Michael Freyberg, Natalie A. Webb, Simon Rosen, Masaaki Sakano, D. Law-Green, G. Denkinson, Axel Schwope, P. Esquej, A. E. Scott, Vladimir Yershov, Laurent Michel, M. J. Page, Jean Ballet, María Teresa Ceballos, Georg Lamer, R. D. Saxton, John P. Pye, Sean Farrell, R. Della Ceca, Valentina Braito, Francisco J. Carrera, Fabien Grisé, Mickael Coriat, Christian Motch, Didier Barret, P. Rodriguez, Dacheng Lin, K. L. Page, Clive G. Page, M. G. Watson, Richard Sturm, Patrick Guillout, A. M. Read, A. Nebot Gomez-Moran, L. Heil, Ivan Zolotukhin, R. Martino
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 590, pp.A1. ⟨10.1051/0004-6361/201526416⟩
Astronomy and Astrophysics-A&A, 2016, 590, pp.A1. ⟨10.1051/0004-6361/201526416⟩
Astron.Astrophys.
Astron.Astrophys., 2016, 590, pp.A1. ⟨10.1051/0004-6361/201526416⟩
Astron.Astrophys., 2016, 590, pp.A1. 〈10.1051/0004-6361/201526416〉
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 590, pp.A1. ⟨10.1051/0004-6361/201526416⟩
Astronomy and Astrophysics-A&A, 2016, 590, pp.A1. ⟨10.1051/0004-6361/201526416⟩
Astron.Astrophys.
Astron.Astrophys., 2016, 590, pp.A1. ⟨10.1051/0004-6361/201526416⟩
Astron.Astrophys., 2016, 590, pp.A1. 〈10.1051/0004-6361/201526416〉
Thanks to the large collecting area (3 x ~1500 cm$^2$ at 1.5 keV) and wide field of view (30' across in full field mode) of the X-ray cameras on board the European Space Agency X-ray observatory XMM-Newton, each individual pointing can result in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::971afe1aca26200cf224285287c71037
https://hal.archives-ouvertes.fr/hal-01554183
https://hal.archives-ouvertes.fr/hal-01554183
Autor:
Frédéric Arenou, Patrick Guillout, A. Nebot Gomez-Moran, Tsevi Mazeh, Caroline Soubiran, J.-B. Salomon, Yveline Lebreton, Jean-Louis Halbwachs, Dimitri Pourbaix, Lev Tal-Or, Benoit Famaey, Flavien Kiefer
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, 2016, 458 (3), pp.3272-3281. ⟨10.1093/mnras/stw545⟩
Monthly Notices of the Royal Astronomical Society, 2016, 458 (3), pp.3272-3281. ⟨10.1093/mnras/stw545⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 458 (3), pp.3272-3281. ⟨10.1093/mnras/stw545⟩
Monthly Notices of the Royal Astronomical Society, 2016, 458 (3), pp.3272-3281. ⟨10.1093/mnras/stw545⟩
In anticipation of the Gaia astrometric mission, a large sample of spectroscopic binaries has been observed since 2010 with the SOPHIE spectrograph at the Haute--Provence Observatory. Our aim is to derive the orbital elements of double-lined spectros
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12cc2b463566d0436add3b7368a9fa2e
https://hal.archives-ouvertes.fr/hal-01291148/document
https://hal.archives-ouvertes.fr/hal-01291148/document
Autor:
Tsevi Mazeh, H. M. J. Boffin, Dimitri Pourbaix, A. Nebot Gomez-Moran, Lev Tal-Or, J. L. Halbwachs, Flavien Kiefer, Patrick Guillout, Frédéric Arenou, J.-B. Le Bouquin, Hugues Sana, Alain Jorissen, S Guieu, Yveline Lebreton, J.-B. Salomon, R. Grellmann, F. Anthonioz, Benoit Famaey
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, 2016, 455 (3), pp.3303-3311. ⟨10.1093/mnras/stv2497⟩
Monthly Notices of the Royal Astronomical Society, 2016, 455 (3), pp.3303-3311. ⟨10.1093/mnras/stv2497⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 455 (3), pp.3303-3311. ⟨10.1093/mnras/stv2497⟩
Monthly Notices of the Royal Astronomical Society, 2016, 455 (3), pp.3303-3311. ⟨10.1093/mnras/stv2497⟩
In anticipation of the Gaia astrometric mission, a sample of spectroscopic binaries is being observed since 2010 with the Sophie spectrograph at the Haute--Provence Observatory. Our aim is to derive the orbital elements of double-lined spectroscopic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0100d108b9377f492e581fc290643459
https://hal.archives-ouvertes.fr/hal-01255808
https://hal.archives-ouvertes.fr/hal-01255808
Autor:
E. Marilli, Antonio Frasca, A. Klutsch, Patrick Guillout, G. Mignemi, R. Freire Ferrero, Katia Biazzo
Publikováno v:
Astronomy & Astrophysics. 490:737-742
During the study of a large set of late-type stellar X-ray sources, we discovered a large fraction of multiple systems. In this paper we investigate the orbital elements and kinematic properties of three new spectroscopic triple systems as well as sp
Autor:
J. L. Halbwachs, Tsevi Mazeh, Frédéric Arenou, Patrick Guillout, Yveline Lebreton, Benoit Famaey, Dimitri Pourbaix, Lev Tal-Or, J.-B. Salomon, Rodrigo A. Ibata
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2014, 445 (3), pp.2371-2377. ⟨10.1093/mnras/stu1838⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 445 (3), pp.2371-2377. ⟨10.1093/mnras/stu1838⟩
Monthly Notices of the Royal Astronomical Society, 2014, 445 (3), pp.2371-2377. ⟨10.1093/mnras/stu1838⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 445 (3), pp.2371-2377. ⟨10.1093/mnras/stu1838⟩
In anticipation of the Gaia astrometric mission, a large sample of spectroscopic binaries is being observed since 2010 with the Sophie spectrograph at the Haute--Provence Observatory. Our aim is to derive the orbital elements of double-lined spectros
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e8281ed16f673dc56f4776680f798b2
https://hal.science/hal-01094503
https://hal.science/hal-01094503
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, ⟨10.1051/0004-6361/201322718⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, ⟨10.1051/0004-6361/201322718⟩
Ou4 is a recently discovered bipolar outflow with a projected size of more than one degree in the plane of the sky. It is apparently centred on the young stellar cluster -whose most massive representative is the triple system HR8119- inside the HII r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d265b046536d5fbf7d1fab58f7e2ca4f
Autor:
Ignacio Negueruela, Natalie A. Webb, Mark Cropper, Christian Motch, Francisco J. Carrera, Simon Rosen, F. X. Pineau, R. S. Warwick, Jonathan Tedds, Axel Schwope, M. W. Pakull, Patrick Guillout, M. G. Watson
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics, 2010, 523, A92
instname
Astronomy and Astrophysics, 2010, 523, A92
We report the results of an optical campaign carried out by the XMM-Newton Survey Science Centre with the specific goal of identifying the brightest X-ray sources in the XMM-Newton Galactic plane survey. In addition to photometric and spectroscopic o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::acac3785b4a139fcdb3b5c144668344b
http://hdl.handle.net/10261/46856
http://hdl.handle.net/10261/46856