Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Colin P. Folsom"'
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 1, p L22 (2024)
Dynamically active planetary systems orbit a significant fraction of white dwarf stars. These stars often exhibit surface metals accreted from debris disks, which are detected through infrared excess or transiting structures. However, the full journe
Externí odkaz:
https://doaj.org/article/131a290cce9e4485a12bf7d312ea4b54
KELT-9b is an ultra-hot Jupiter observed to be undergoing extreme mass loss. Its A0-type host star has a radiative envelope, which makes its surface layers prone to retaining recently accreted material. To search for potential signs of planetary mate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ea73121f059af1662a89fb0c244f2fb
Autor:
Colin P. Folsom, Mihkel Kama, Tõnis Eenmäe, Indrek Kolka, Anna Aret, Vitalii Checha, Anni Kasikov, Laurits Leedjärv, Heleri Ramler
Context: Few exoplanets around hot stars with radiative envelopes have been discovered, although new observations from the TESS mission are improving this. Stars with radiative envelopes have little mixing at their surface, and thus their surface abu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f9906cbab12d8cc42a951555361326f
http://arxiv.org/abs/2111.07526
http://arxiv.org/abs/2111.07526
Autor:
Colin P. Folsom, Pascal Petit, Julien Morin, Claire Moutou, Gaitee A. J. Hussain, Andres Carmona, Xavier Delfosse, Stefano Bellotti
Stellar activity limits the radial velocity search and characterisation of exoplanets, as it introduces spurious jitter in the data sets and prevents the correct retrieval of a planetary signal. This is key for M dwarfs, considering that they manifes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32eb2d3b62f1c68da24b03e804310bef
http://arxiv.org/abs/2110.10633
http://arxiv.org/abs/2110.10633
Publikováno v:
Proceedings of the International Astronomical Union. 15:181-184
Young solar analogs reaching the main sequence experience very strong magnetic activity, directly linked to their angular momentum loss through wind and mass ejections. We investigate here the surface and chromospheric activity of the ultra-rapid rot
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
Autor:
Colin P. Folsom, Jean-François Donati, Renada Konstantinova-Antova, Gregg A. Wade, Pascal Petit, O. Espagnet, Corinne Charbonnel, P. Mathias, Michel Aurière, Thierry Roudier
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A130. ⟨10.1051/0004-6361/202039573⟩
Astronomy and Astrophysics-A&A, 2021, 646, pp.A130. ⟨10.1051/0004-6361/202039573⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A130. ⟨10.1051/0004-6361/202039573⟩
Astronomy and Astrophysics-A&A, 2021, 646, pp.A130. ⟨10.1051/0004-6361/202039573⟩
Context: Pollux is considered as an archetype of a giant star hosting a planet. We then discovered a weak magnetic field at its surface using spectropolarimetry. Aims and Methods: We followed up our investigations on Pollux first using ESPaDOnS at CF
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74bda7b4a795c45649496f393884017c
https://hal.archives-ouvertes.fr/hal-03146215/file/aa39573-20.pdf
https://hal.archives-ouvertes.fr/hal-03146215/file/aa39573-20.pdf
Autor:
Luisa Rebull, Evelyne Alecian, Jean-François Donati, K. N. Grankin, Ann Marie Cody, K. Pouilly, Jerome Bouvier, Silvia H. P. Alencar, Colin P. Folsom
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 656, pp.A50. ⟨10.1051/0004-6361/202140850⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 656, pp.A50. ⟨10.1051/0004-6361/202140850⟩
Astronomy and Astrophysics-A&A, EDP Sciences, In press
Astronomy and Astrophysics-A&A, 2021, ⟨10.1051/0004-6361/202140850⟩
HAL
Astronomy and Astrophysics-A&A, 2021, 656, pp.A50. ⟨10.1051/0004-6361/202140850⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 656, pp.A50. ⟨10.1051/0004-6361/202140850⟩
Astronomy and Astrophysics-A&A, EDP Sciences, In press
Astronomy and Astrophysics-A&A, 2021, ⟨10.1051/0004-6361/202140850⟩
HAL
We aim to characterize the magnetospheric accretion process in the young stellar object V807 Tau, one of the most stable dippers revealed by K2 in the Taurus star forming region. We performed photometric and spectropolarimetric follow-up observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::427b4444e7ad95c8ef8bda47a3ed55b6
Autor:
Coralie Neiner, Aline A. Vidotto, Gregg Hallinan, Colin P. Folsom, D. Ó Fionnagáin, Pascal Petit, Ward B. Manchester
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 500, pp.3438-3453. ⟨10.1093/mnras/staa3468⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500, pp.3438-3453. ⟨10.1093/mnras/staa3468⟩
We investigate the wind of lambda And, a solar-mass star that has evolved off the main sequence becoming a sub-giant. We present spectropolarimetric observations and use them to reconstruct the surface magnetic field of lambda And. Although much olde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e89cff4316fa75a342155bf7d0c6c11
https://resolver.caltech.edu/CaltechAUTHORS:20210202-103629939
https://resolver.caltech.edu/CaltechAUTHORS:20210202-103629939
Autor:
B. Zaire, Colin P. Folsom, X. Delfosse, E. Hébrard, Baptiste Klein, Jean-François Donati, Xavier Bonfils, Julien Morin
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, 500 (2), pp.1844-1850. ⟨10.1093/mnras/staa3396⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500 (2), pp.1844-1850. ⟨10.1093/mnras/staa3396⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, ⟨10.1093/mnras/staa3396⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (2), pp.1844-1850. ⟨10.1093/mnras/staa3396⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500 (2), pp.1844-1850. ⟨10.1093/mnras/staa3396⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, ⟨10.1093/mnras/staa3396⟩
We report the detection of a large-scale magnetic field at the surface of the slowly-rotating fully-convective M dwarf Proxima Centauri. Ten circular polarization spectra, collected from April to July 2017 with the HARPS-Pol spectropolarimeter, exhib
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24773bb2f5d520c0ff1b0fea6d7143d4
https://hal.archives-ouvertes.fr/hal-02996801
https://hal.archives-ouvertes.fr/hal-02996801