Search Results - "BOHLENDER, D"
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The MiMeS survey of Magnetism in Massive Stars: magnetic analysis of the O-type stars
Published in Monthly notices of the Royal Astronomical Society (01-02-2017)“…We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the framework of the Magnetism in Massive Stars (MiMeS) Survey…”
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The magnetic early B-type stars I: magnetometry and rotation
Published in Monthly notices of the Royal Astronomical Society (2018)“…Abstract The rotational and magnetic properties of many magnetic hot stars are poorly characterized, therefore the Magnetism in Massive Stars and Binarity and…”
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The magnetic early B-type stars – III. A main-sequence magnetic, rotational, and magnetospheric biography
Published in Monthly notices of the Royal Astronomical Society (21-11-2019)“…Magnetic confinement of stellar winds leads to the formation of magnetospheres, which can be sculpted into centrifugal magnetospheres (CMs) by rotational…”
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The MiMeS survey of magnetism in massive stars: introduction and overview
Published in Monthly notices of the Royal Astronomical Society (11-02-2016)“…The MiMeS (Magnetism in Massive Stars) project is a large-scale, high-resolution, sensitive spectropolarimetric investigation of the magnetic properties of O-…”
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The magnetic early B-type stars – IV. Breakout or leakage? H α emission as a diagnostic of plasma transport in centrifugal magnetospheres
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT Rapidly rotating early-type stars with strong magnetic fields frequently show H α emission originating in centrifugal magnetospheres (CMs),…”
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MOBSTER – VI. The crucial influence of rotation on the radio magnetospheres of hot stars
Published in Monthly notices of the Royal Astronomical Society (29-04-2022)“…ABSTRACT Numerous magnetic hot stars exhibit gyrosynchrotron radio emission. The source electrons were previously thought to be accelerated to relativistic…”
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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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GAS-PHASE ABSORPTIONS OF C + 60 : A NEW COMPARISON WITH ASTRONOMICAL MEASUREMENTS
Published in The Astrophysical journal (10-11-2016)“…Campbell et al. recently revised, by a few tenths of an Å, the wavelengths for their low-temperature laboratory measurements of fullerene bands. This accounts…”
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HD 35502: a hierarchical triple system with a magnetic B5IVpe primary
Published in Monthly notices of the Royal Astronomical Society (01-08-2016)“…We present our analysis of HD 35502 based on high- and medium-resolution spectropolarimetric observations. Our results indicate that the magnetic B5IVsnp star…”
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A magnetic confinement versus rotation classification of massive-star magnetospheres
Published in Monthly notices of the Royal Astronomical Society (11-02-2013)“…Building on results from the Magnetism in Massive Stars (MiMeS) project, this paper shows how a two-parameter classification of massive-star magnetospheres in…”
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Analysis of Eight Magnetic Chemically Peculiar Stars With Rotational Modulation
Published in Monthly notices of the Royal Astronomical Society (10-11-2022)“…Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar photometry to the astronomical community. We have used TESS data…”
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Confirming HD 23478 as a new magnetic B star hosting an Hα-bright centrifugal magnetosphere
Published in Monthly notices of the Royal Astronomical Society (01-08-2015)“…In this paper, we report 23 magnetic field measurements of the B3IV star HD 23478: 12 obtained from high-resolution Stokes V spectra using the ESPaDOnS…”
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HR5907: Discovery of the most rapidly rotating magnetic early B-type star by the MiMeS Collaboration[dagger]
Published in Monthly notices of the Royal Astronomical Society (01-01-2012)“…ABSTRACT We report the discovery and analysis of a very strong magnetic field in the rapidly rotating early B-type star HR5907, based on observations obtained…”
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Hot Jupiters and Hot Spots: The Short- and Long-Term Chromospheric Activity on Stars with Giant Planets
Published in The Astrophysical journal (01-04-2005)“…We monitored the chromospheric activity in the Ca II H and K lines of 13 solar-type stars (including the Sun): 8 of them over 3 years at the…”
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The surface magnetic field and chemical abundance distributions of the B2V helium-strong star HD 184927
Published in Monthly notices of the Royal Astronomical Society (21-02-2015)“…A new time series of high-resolution Stokes I and V spectra of the magnetic B2V star HD 184927 has been obtained in the context of the Magnetism in Massive…”
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Identification of H2CCC as a Diffuse Interstellar Band Carrier
Published in The Astrophysical journal (01-01-2011)“…We present strong evidence that the broad, diffuse interstellar bands (DIBs) at 4881 and 5450 A are caused by the B 1 B 1 arrow left X 1 A 1 transition of…”
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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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A magnetic confinement versus rotation classification of massive-star magnetospheres
Published in Monthly notices of the Royal Astronomical Society (11-02-2013)Get full text
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Magnetic field, differential rotation and activity of the hot-Jupiter-hosting star HD 179949
Published in Monthly notices of the Royal Astronomical Society (01-06-2012)“…HD 179949 is an F8V star, orbited by a giant planet at ∼8 R ★ every 3.092 514 d. The system was reported to undergo episodes of stellar activity enhancement…”
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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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