Search Results - "Thizy, O"
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Multisite spectroscopic seismic study of the β Cep star V2052 Ophiuchi: inhibition of mixing by its magnetic field
Published in Monthly notices of the Royal Astronomical Society (21-11-2012)“…ABSTRACT We used extensive ground‐based multisite and archival spectroscopy to derive observational constraints for a seismic modelling of the magnetic β Cep…”
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On the incidence of magnetic fields in slowly pulsating B, β Cephei and B-type emission-line stars
Published in Monthly notices of the Royal Astronomical Society (21-09-2009)“…We have obtained 40 high-resolution circular spectropolarimetric measurements of 12 slowly pulsating B (SPB) stars, eight β Cephei stars and two Be stars with…”
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Evolution of the disk of π Aqr: From near-disappearance to a strong maximum
Published in New astronomy (01-11-2019)“…•The disk surrounding the primary component of π Aqr nearly disappeared in early 2014.•The disk has slowly recovered, now reaching strengths not seen in three…”
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THE 2011 PERIASTRON PASSAGE OF THE Be BINARY δ Scorpii
Published in The Astrophysical journal (01-04-2013)“…We describe the results of the world-wide observing campaign of the highly eccentric Be binary system delta Scorpii 2011 periastron passage which involved…”
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THE 2011 PERIASTRON PASSAGE OF THE Be BINARY {delta} Scorpii
Published in The Astrophysical journal (01-04-2013)“…We describe the results of the world-wide observing campaign of the highly eccentric Be binary system {delta} Scorpii 2011 periastron passage which involved…”
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Multisite spectroscopic seismic study of the [beta] Cep star V2052 Ophiuchi: inhibition of mixing by its magnetic field
Published in Monthly notices of the Royal Astronomical Society (21-11-2012)“…We used extensive ground-based multisite and archival spectroscopy to derive observational constraints for a seismic modelling of the magnetic [beta] Cep star…”
Get full text
Journal Article -
8
On the incidence of magnetic fields in slowly pulsating B, β Cephei and B-type emission-line stars
Published in Monthly notices of the Royal Astronomical Society (21-09-2009)Get full text
Journal Article -
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On the incidence of magnetic fields in slowly pulsating B, b Cephei and B-type emission-line stars
Published in Monthly notices of the Royal Astronomical Society (21-09-2009)“…We have obtained 40 high-resolution circular spectropolarimetric measurements of 12 slowly pulsating B (SPB) stars, eight b Cephei stars and two Be stars with…”
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Journal Article -
10
On the incidence of magnetic fields in slowly pulsating B, [beta] Cephei and B-type emission-line stars
Published in Monthly notices of the Royal Astronomical Society (01-09-2009)“…We have obtained 40 high-resolution circular spectropolarimetric measurements of 12 slowly pulsating B (SPB) stars, eight [beta] Cephei stars and two Be stars…”
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Organizing a professional–amateur collaboration with a Lhires III spectrograph
Published in Planetary and space science (01-11-2008)“…Amateur spectroscopists are getting organized to contribute to professional astronomy work. We present here the work done within the AUDE association to…”
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Evolution of the disk of pi Aqr: from near-disappearance to a strong maximum
Published 21-06-2019“…New Astronomy (vol 73, id 101279, 2019) Some Be stars display important variability of the strength of the emission lines formed in their disk. This is notably…”
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Thermal properties of slowly rotating asteroids: Results from a targeted survey
Published 15-05-2019“…A&A 625, A139 (2019) Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat…”
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High cadence measurement of neutral sodium and potassium absorption during the 2009-2011 eclipse of epsilon Aurigae
Published 28-06-2012“…2012, J. Amer. Assoc. Var. Star Obs., 40, 729 The results of a spectroscopic survey of epsilon Aurigae during eclipse using a network of small telescopes are…”
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The 2011 Periastron Passage of the Be Binary delta Scorpii
Published 17-02-2013“…We describe the results of the world-wide observing campaign of the highly eccentric Be binary system delta Scorpii 2011 periastron passage which involved…”
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Multisite spectroscopic seismic study of the beta Cep star V2052 Oph: inhibition of mixing by its magnetic field
Published 21-08-2012“…We used extensive ground-based multisite and archival spectroscopy to derive observational constraints for a seismic modelling of the magnetic beta Cep star…”
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On the incidence of magnetic fields in slowly-pulsating B, Beta Cephei and B-type emission line stars
Published 08-06-2009“…We have obtained 40 high-resolution circular spectropolarimetric measurements of 12 slowly-pulsating B (SPB) stars, 8 Beta Cephei stars and two Be stars with…”
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The magnetic field of the B3V star 16 Pegasi
Published 25-12-2008“…The Slowly Pulsating B3V star 16 Pegasi was discovered by Hubrig (2006) to be magnetic, based on low-resolution spectropolarimetric observations with FORS1 at…”
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