Zobrazeno 1 - 10
of 70
pro vyhledávání: '"Stephane Guilloteau"'
Autor:
Ya-Wen Tang, Anne Dutrey, Patrick M. Koch, Stephane Guilloteau, Hsi-Wei Yen, Emmanuel di Folco, Eric Pantin, Takayuki Muto, Akimasa Kataoka, Robert Brauer
Publikováno v:
The Astrophysical Journal Letters, Vol 947, Iss 1, p L5 (2023)
We report Atacama Large Millimeter/submillimeter Array (ALMA) polarization observations at 3 and 0.9 mm toward the GG Tau A system. In the ring, the percentage is relatively homogeneous at 3 mm, being 1.2%, while it exhibits a clear radial variation
Externí odkaz:
https://doaj.org/article/208bd350511346fdbb8d242f292ee0b4
Autor:
Emmanuel Di Folco, Anthony Boccaletti, Anne Dutrey, Ya-Wen Tang, Stephane Guilloteau, Eric Pantin
AB Aur is a bright and young Herbig Ae star surrounded by a broad transitional disk, with a long record of detailed observations at various wavelengths. Multiple direct and indirect evidences for the presence of embedded proto-planets have been repor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4bb1e4331104602b86000480ef4d05c4
https://hal.science/hal-03838445
https://hal.science/hal-03838445
Autor:
Edwin A. Bergin, Anne Dutrey, Richard Teague, Thomas Henning, Wouter Vlemmings, Stephane Guilloteau, Dmitry Semenov, Rolf Kuiper, Charles L. H. Hull, Ian W. Stephens
We report observations of polarized line and continuum emission from the disk of TW~Hya using the Atacama Large Millimeter/submillimeter Array. We target three emission lines, $^{12}$CO (3-2), $^{13}$CO (3-2) and CS (7-6), to search for linear polari
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9e9fa3d0d7b606ed5efa686d642d7b8
http://arxiv.org/abs/2109.09247
http://arxiv.org/abs/2109.09247
Autor:
Dmitry Semenov, Cecile Favre, Davide Fedele, Richard Teague, Anne Dutrey, Stephane Guilloteau, Thomas Henning, Grigorii Smirnov-Pinchukov
We performed a deep search for CCS, SO, SO2, OCS, H2S, H2CS and other molecules in the DM Tau protoplanetary disk at 2mm with PolyFiX@NOEMA. With a beam of ~2''x1'' and a spectral resolution of 0.3 km/s, a high sensitivity of ~3.8 mJy/beam was achiev
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b71f02724e0cc88f936bfe4974a6c7dd
https://doi.org/10.5194/epsc2020-304
https://doi.org/10.5194/epsc2020-304
Autor:
E. Chapillon, J. C. Augereau, Anthony Boccaletti, Stephane Guilloteau, Anne Dutrey, Vincent Piétu, J. Péricaud, E. Di Folco
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A94. ⟨10.1051/0004-6361/201732243⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A94. ⟨10.1051/0004-6361/201732243⟩
Context.The study of gas-rich debris discs is fundamental to characterising the transition between protoplanetary discs and debris discs.Aims.We determine the physical parameters of the brightest gas-rich debris disc orbiting HD 141569A.Methods.We an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5031f1861abd29619dfc1a815de8e148
https://hal.sorbonne-universite.fr/hal-02553367/document
https://hal.sorbonne-universite.fr/hal-02553367/document
Autor:
Richard Teague, Aurora Sicilia-Aguilar, L. Chen, Mario Flock, Anne Dutrey, F. Cruz-Sáenz de Miera, Kundan Kadam, Jacob Aaron White, Antonio Hales, D. Semenov, Ágnes Kóspál, Andrea Banzatti, Th. Henning, Péter Ábrahám, Vitaly Akimkin, Eduard I. Vorobyov, A. G. Hughes, Stephane Guilloteau
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2020, 904 (1), pp.37. ⟨10.3847/1538-4357/abbb94⟩
The Astrophysical Journal, American Astronomical Society, 2020, 904 (1), pp.37. ⟨10.3847/1538-4357/abbb94⟩
Extreme outbursts in young stars may be a common stage of pre-main-sequence stellar evolution. These outbursts, caused by enhanced accretion and accompanied by increased luminosity, can also strongly impact the evolution of the circumstellar environm
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, 497 (4), pp.4276-4281. ⟨10.1093/mnras/staa2308⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 497 (4), pp.4276-4281. ⟨10.1093/mnras/staa2308⟩
International audience; The HCO+ and DCO+ molecules are commonly used as tracers in the interstellar medium. Therefore, accurate rotational rate coefficients of these systems with He and H2 are crucial in non-local thermal equilibrium models. We dete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3696a7f5d965af1dc6ef0b2047203a97
https://hal-cnrs.archives-ouvertes.fr/hal-03044185
https://hal-cnrs.archives-ouvertes.fr/hal-03044185
Autor:
W. Iqbal, Valentine Wakelam, E. Chapillon, Audrey Coutens, Stephane Guilloteau, Anne Dutrey, Liton Majumdar
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, 2019, 484 (2), pp.1563-1573. ⟨10.1093/mnras/stz068⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 484 (2), pp.1563-1573. ⟨10.1093/mnras/stz068⟩
Protoplanetary disks are challenging objects for astrochemical models due to strong density and temperature gradients and due to the UV photons 2D propagation. In this paper, we have studied the importance of several model parameters on the predicted
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a6b30f46149a92833bcf6e0e3595084
https://hal.archives-ouvertes.fr/hal-01981366
https://hal.archives-ouvertes.fr/hal-01981366
Autor:
Gail Schaefer, Vincent Piétu, E. Chapillon, Nicolas Grosso, Stephane Guilloteau, E. Di Folco, Anne Dutrey, Tracy L. Beck, Lisa Prato, Gregory A. Feiden, Michal Simon
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2019, 884 (1), pp.id. 42. ⟨10.3847/1538-4357/ab3e3b⟩
The Astrophysical Journal, American Astronomical Society, 2019, 884 (1), pp.id. 42. ⟨10.3847/1538-4357/ab3e3b⟩
The Astrophysical Journal, 2019, 884 (1), pp.id. 42. ⟨10.3847/1538-4357/ab3e3b⟩
The Astrophysical Journal, American Astronomical Society, 2019, 884 (1), pp.id. 42. ⟨10.3847/1538-4357/ab3e3b⟩
The accuracy of masses of pre-main sequence (PMS) stars derived from their locations on the Hertzsprung-Russell Diagram (HRD) can be tested by comparison with accurate and precise masses determined independently. We present 29 single stars in the Tau
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7783a5e1f4cf1ac24e2117a211ef12e8
http://hdl.handle.net/20.500.12278/95338
http://hdl.handle.net/20.500.12278/95338
Autor:
Cécile Favre, Franck Hersant, Richard Teague, Anne Dutrey, Vincent Piétu, Th. Henning, D. Semenov, Davide Fedele, Stephane Guilloteau, Edwige Chapillon
Publikováno v:
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 617, pp.id.A28. ⟨10.1051/0004-6361/201832980⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 617, pp.id.A28. ⟨10.1051/0004-6361/201832980⟩
Context. Several sulfur-bearing molecules are observed in the interstellar medium and in comets, in strong contrast to protoplanetary disks where only CS, H$_2$CS and SO have been detected so far. Aims. We combine observations and chemical models to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47a14f576b3ae6f412058f30a5d7bfcf
http://hdl.handle.net/20.500.12278/95552
http://hdl.handle.net/20.500.12278/95552