Search Results - "Farès, R."
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Magnetospheric accretion and spin-down of the prototypical classical T Tauri star AA Tau
Published in Monthly notices of the Royal Astronomical Society (21-12-2010)“…From observations collected with the ESPaDOnS spectropolarimeter at the Canada–France–Hawaii Telescope (CFHT) and with the NARVAL spectropolarimeter at the…”
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2
Magnetic cycles of the planet-hosting star τ Bootis
Published in Monthly notices of the Royal Astronomical Society (11-04-2008)“…We have obtained new spectropolarimetric observations of the planet-hosting star τ Bootis, using the ESPaDOnS and NARVAL spectropolarimeters at the…”
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Magnetic cycles of the planet-hosting star τ Bootis – II. A second magnetic polarity reversal
Published in Monthly notices of the Royal Astronomical Society (21-09-2009)“…In this paper, we present new spectropolarimetric observations of the planet-hosting star τ Bootis, using ESPaDOnS and Narval spectropolarimeters at…”
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4
A study of the magnetic activity and variability of GJ 436
Published in Monthly notices of the Royal Astronomical Society (30-11-2022)“…ABSTRACT We present a magnetic activity study of GJ 436 using spectroscopic data from HARPS, spanning over 14 yr, and additional data from NARVAL, falling…”
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5
Planets and stellar activity: hide and seek in the CoRoT-7 system
Published in Monthly notices of the Royal Astronomical Society (21-09-2014)“…Since the discovery of the transiting super-Earth CoRoT-7b, several investigations have yielded different results for the number and masses of planets present…”
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6
Optimal entropy generation in Darcy-Forchheimer magnetized flow in a square enclosure filled with silver based water nanoliquid
Published in Journal of thermal analysis and calorimetry (01-01-2022)“…Current communication candidly explicates the incremental aspect of generated entropy in apermeablesquare enclosure. Porosity aspects are mathematically…”
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On the environment surrounding close-in exoplanets
Published in Monthly notices of the Royal Astronomical Society (01-06-2015)“…Exoplanets in extremely close-in orbits are immersed in a local interplanetary medium (i.e. the stellar wind) much denser than the local conditions encountered…”
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A BCool magnetic snapshot survey of solar-type stars
Published in Monthly notices of the Royal Astronomical Society (11-11-2014)“…We present the results of a major high-resolution spectropolarimetric BCool project magnetic survey of 170 solar-type stars. Surface magnetic fields were…”
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The Sun as a planet-host star: proxies from SDO images for HARPS radial-velocity variations
Published in Monthly notices of the Royal Astronomical Society (01-04-2016)“…The Sun is the only star whose surface can be directly resolved at high resolution, and therefore constitutes an excellent test case to explore the physical…”
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A small survey of the magnetic fields of planet-host stars
Published in Monthly notices of the Royal Astronomical Society (21-10-2013)“…Using spectropolarimetry, we investigate the large-scale magnetic topologies of stars hosting close-in exoplanets. A small survey of 10 stars has been done…”
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Stellar magnetism: empirical trends with age and rotation
Published in Monthly notices of the Royal Astronomical Society (01-07-2014)“…We investigate how the observed large-scale surface magnetic fields of low-mass stars (∼0.1–2 M⊙), reconstructed through Zeeman–Doppler imaging, vary with age…”
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MOVES – IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT Hot Jupiters provide valuable natural laboratories for studying potential contributions of high-energy radiation to pre-biotic synthesis in the…”
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13
Exoplanet transit variability: bow shocks and winds around HD 189733b
Published in Monthly notices of the Royal Astronomical Society (11-12-2013)“…By analogy with the Solar system, it is believed that stellar winds will form bow shocks around exoplanets. For hot Jupiters the bow shock will not form…”
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Enhancement of dissolution and oral bioavailability of lacidipine via pluronic P123/F127 mixed polymeric micelles: formulation, optimization using central composite design and in vivo bioavailability study
Published in Drug delivery (01-01-2018)“…This study aims at preparing and optimizing lacidipine (LCDP) polymeric micelles using thin film hydration technique in order to overcome LCDP…”
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MOVES – II. Tuning in to the radio environment of HD189733b
Published in Monthly notices of the Royal Astronomical Society (01-06-2019)“…ABSTRACT We present stellar wind modelling of the hot Jupiter host HD189733, and predict radio emission from the stellar wind and the planet, the latter…”
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Searching for star–planet interactions within the magnetosphere of HD 189733
Published in Monthly notices of the Royal Astronomical Society (21-07-2010)“…HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study magnetospheric interactions between the star and the planet, we…”
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The connection between stellar activity cycles and magnetic field topology
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)“…Zeeman–Doppler imaging (ZDI) has successfully mapped the large-scale magnetic fields of stars over a large range of spectral types, rotation periods and ages…”
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MOVES – V. Modelling star–planet magnetic interactions of HD 189733
Published in Monthly notices of the Royal Astronomical Society (07-04-2022)“…ABSTRACT Magnetic interactions between stars and close-in planets may lead to a detectable signal on the stellar disc. HD 189733 is one of the key exosystems…”
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A risk assessment model for transfusion transmission of dengue
Published in Letters in applied microbiology (01-11-2022)“…Dengue virus (DENV) is a disease‐causing agent normally transmitted from person to person through the bite of an infected mosquito. In addition to…”
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The stellar wind cycles and planetary radio emission of the t Boo system
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…t Boo is an intriguing planet-host star that is believed to undergo magnetic cycles similar to the Sun, but with a duration that is about one order of…”
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