Zobrazeno 1 - 10
of 166
pro vyhledávání: '"Moira Jardine"'
Autor:
Moira Jardine, Rose Waugh
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:5465-5477
Magnetic confinement of dense plasma is found in the magnetospheres of both high- and low-mass stars. Trapped material traces the magnetic field structure, often at large distances from the star where the magnetic structure is otherwise difficult to
One of the puzzles to have emerged from the Kepler and TESS missions is the existence of unexplained dips in the lightcurves of a small fraction of rapidly-rotating M dwarfs in young open clusters and star-forming regions. We present a theoretical in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::893c55587615d8edd9245115fd39ab64
http://arxiv.org/abs/2211.04765
http://arxiv.org/abs/2211.04765
Autor:
Moira Jardine, Sarah Faller
Observations of rapidly-rotating cool stars often show coronal slingshot prominences that remove mass and angular momentum when they are ejected. The derived masses of these prominences show a scatter of some two orders of magnitude. In order to inve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed3ded89d09efdfa9fbc9e21a8574ca6
http://arxiv.org/abs/2205.06681
http://arxiv.org/abs/2205.06681
Autor:
C. Moutou, Pascal Fouqué, L. Lehmann, X. Delfosse, S. H. P. Alencar, B. Finociety, Jerome Bouvier, René Doyon, J.-F. Donati, B. Zaire, L. Yu, Baptiste Klein, Guillaume Hébrard, K. N. Grankin, Francois Menard, Étienne Artigau, Moira Jardine, Ágnes Kóspál
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, 2021, 508 (3), pp.3427-3445. ⟨10.1093/mnras/stab2778⟩
Monthly Notices of the Royal Astronomical Society, 2021, 508 (3), pp.3427-3445. ⟨10.1093/mnras/stab2778⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 508 (3), pp.3427-3445. ⟨10.1093/mnras/stab2778⟩
Monthly Notices of the Royal Astronomical Society, 2021, 508 (3), pp.3427-3445. ⟨10.1093/mnras/stab2778⟩
We report results of a spectropolarimetric and photometric monitoring of the weak-line T Tauri star V410 Tau based on data collected mostly with SPIRou, the near-infrared (NIR) spectropolarimeter recently installed at the Canada-France-Hawaii Telesco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::acb4bd65774db442aecbbe653a738258
https://hal.archives-ouvertes.fr/hal-03433075
https://hal.archives-ouvertes.fr/hal-03433075
Autor:
Brian E. Wood, Seth Redfield, Hunter Vannier, Jeffrey L. Linsky, Moira Jardine, Fallon Konow, Hans-Reinhard Müller, Julián D. Alvarado-Gómez, Allison Youngblood, Jeremy J. Drake, Aline A. Vidotto
High resolution UV spectra of stellar H I Lyman-alpha lines from the Hubble Space Telescope (HST) provide observational constraints on the winds of coronal main sequence stars, thanks to an astrospheric absorption signature created by the interaction
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a026f62c2aec1275b670b3e38f2b122d
https://hdl.handle.net/10023/25596
https://hdl.handle.net/10023/25596
Autor:
Vincent Bourrier, Robert D. Kavanagh, Joe Llama, Aline A. Vidotto, Christiane Helling, D. Ó Fionnagáin, Rim Fares, C. Moutou, Moira Jardine, Peter J. Wheatley
Publikováno v:
Proceedings of the International Astronomical Union. 15:305-309
The hot Jupiter HD189733b is expected to be a source of strong radio emission, due to its close proximity to its magnetically active host star. Here, we model the stellar wind of its host star, based on reconstructed surface stellar magnetic field ma
Autor:
Robert D. Kavanagh, Baptiste Klein, Aline A. Vidotto, Moira Jardine, Jean-François Donati, Dúalta Ó Fionnagáin
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, 2021, 504 (1), pp.1511-1518. ⟨10.1093/mnras/stab929⟩
Monthly Notices of the Royal Astronomical Society, 2021, 504 (1), pp.1511-1518. ⟨10.1093/mnras/stab929⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 504 (1), pp.1511-1518. ⟨10.1093/mnras/stab929⟩
Monthly Notices of the Royal Astronomical Society, 2021, 504 (1), pp.1511-1518. ⟨10.1093/mnras/stab929⟩
There have recently been detections of radio emission from low-mass stars, some of which are indicative of star-planet interactions. Motivated by these exciting new results, in this paper we present Alfv\'en wave-driven stellar wind models of the two
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5add2cd044eee365d676d4fbe345741
http://arxiv.org/abs/2103.16318
http://arxiv.org/abs/2103.16318
Autor:
Patrick Barth, Moira Jardine, Vincent Bourrier, Nathan J. Mayne, Paul B. Rimmer, Rim Fares, Peter J. Wheatley, Christiane Helling, Eva E. Stüeken, Aline A. Vidotto
Hot Jupiters provide valuable natural laboratories for studying potential contributions of high-energy radiation to prebiotic synthesis in the atmospheres of exoplanets. HD 189733b, a hot Jupiter orbiting a K star, is one of the most studied and best
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b50652f18deb90a8678fa29102b2868a
https://doi.org/10.5194/egusphere-egu21-936
https://doi.org/10.5194/egusphere-egu21-936
Autor:
Rim Fares, Julien Morin, Colin P. Folsom, Alexander Russell, Moira Jardine, Jean-François Donati, Stephen C. Marsden, Sandra V. Jeffers, Victor See, P. Petit, K. Lund
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, 2021, 502 (4), pp.4903-4910. ⟨10.1093/mnras/stab305⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (4), pp.4903-4910. ⟨10.1093/mnras/stab305⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (4), pp.4903-4910. ⟨10.1093/mnras/stab305⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (4), pp.4903-4910. ⟨10.1093/mnras/stab305⟩
The helicity of a magnetic field is a fundamental property that is conserved in ideal MHD. It can be explored in the stellar context by mapping large-scale magnetic fields across stellar surfaces using Zeeman-Doppler imaging. A recent study of 51 sta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5731c51b80e56978daab758cbdfa0b45
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, 2021, 505 (4), pp.5104-5116. ⟨10.1093/mnras/stab1709⟩
Monthly Notices of the Royal Astronomical Society, 2021, 505 (4), pp.5104-5116. ⟨10.1093/mnras/stab1709⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (4), pp.5104-5116. ⟨10.1093/mnras/stab1709⟩
Monthly Notices of the Royal Astronomical Society, 2021, 505 (4), pp.5104-5116. ⟨10.1093/mnras/stab1709⟩
Whilst ``slingshot'' prominences have been observed on M-dwarfs, most if not all theoretical studies have focused on solar-like stars. We present an investigation into stellar prominences around rapidly rotating young M-dwarfs. We have extrapolated t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6dfbd099f82ede10db282400cf7ac38