Search Results - "Smoker, J"
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1
Debris discs with multiple absorption features in metallic lines: circumstellar or interstellar origin?
Published in Monthly notices of the Royal Astronomical Society (11-10-2018)Get full text
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2
A giant outburst two years before the core-collapse of a massive star
Published in Nature (14-06-2007)“…The death of massive stars produces a variety of supernovae, which are linked to the structure of the exploding stars. The detection of several precursor stars…”
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3
A magnetic massive star has experienced a stellar merger
Published in Science (American Association for the Advancement of Science) (12-04-2024)“…Massive stars (those ≥8 solar masses at formation) have radiative envelopes that cannot sustain a dynamo, the mechanism that produces magnetic fields in…”
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4
Distance limits to intermediate- and high-velocity clouds
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…We present optical spectra of 403 stars and quasi-stellar objects in order to obtain distance limits towards intermediate- and high-velocity clouds (IHVCs),…”
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5
Large- and small-scale structure of the intermediate- and high-velocity clouds towards the LMC and SMC
Published in Monthly notices of the Royal Astronomical Society (21-08-2015)“…We employ Ca ii K and Na i D interstellar absorption-line spectroscopy of early-type stars in the Large and Small Magellanic Clouds (LMC, SMC) to investigate…”
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6
A remarkable change of the spectrum of the magnetic Of?p star HD 148937 reveals evidence of an eccentric, high-mass binary
Published in Monthly notices of the Royal Astronomical Society (01-02-2019)“…We report new spectroscopic observations of the magnetic Of?p star HD 148937 obtained since 2015 that differ qualitatively from its extensive historical record…”
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7
Metallicity and Physical Conditions in the Magellanic Bridge
Published in The Astrophysical journal (01-05-2008)“…We present a new analysis of the diffuse gas in the Magellanic Bridge (R.A. [image] 3 super(h)) based on HST STIS E140M and FUSE spectra of two early-type…”
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8
An episode of extremely low precipitable water vapour over Paranal observatory
Published in Monthly notices of the Royal Astronomical Society (21-03-2014)“…We report on an episode of extremely low precipitable water vapour (PWV) of approximately 0.1 mm with a duration of more than 12 h at European Southern…”
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9
Early-type stars observed in the ESO UVES Paranal Observatory Project - III. Sub-parsec and au-scale structure in the interstellar medium
Published in Monthly notices of the Royal Astronomical Society (01-06-2011)“…UVES interstellar observations from the Paranal Observatory Project are presented for early-type stars located in the line of sight to the nearby open clusters…”
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10
Early-type stars observed in the ESO UVES Paranal Observatory Project – IV. Studies of CN, CH+ and CH in the interstellar medium
Published in Monthly notices of the Royal Astronomical Society (21-02-2014)“…High spectral resolution (∼80 000) and signal-to-noise observations from the Ultraviolet and Visual Echelle Spectrograph Paranal Observatory Project (UVES-POP)…”
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11
Early-type stars observed in the ESO UVES Paranal Observatory Project - I. Interstellar Na i UV, Ti ii and Ca ii K observations
Published in Monthly notices of the Royal Astronomical Society (01-04-2006)“…We present an analysis of interstellar Na i (λair= 3302.37 and 3302.98 Å), Ti ii(λair= 3383.76 Å) and Ca ii K (λair= 3933.66 Å) absorption features for 74…”
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12
Macroturbulent and rotational broadening in the spectra of B-type supergiants
Published in Monthly notices of the Royal Astronomical Society (21-10-2002)“…Abstract The absorption-line spectra of early B-type supergiants show significant broadening that implies that an additional broadening mechanism…”
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13
Iron abundances of B-type post-asymptotic giant branch stars in globular clusters: Barnard 29 in M 13 and ROA 5701 in ω Cen
Published in Monthly notices of the Royal Astronomical Society (11-07-2007)“…High-resolution optical and ultraviolet (UV) spectra of two B-type post-asymptotic giant branch (post-AGB) stars in globular clusters, Barnard 29 in M 13 and…”
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14
Ca ii K interstellar observations towards early-type disc and halo stars, abundances and distances of intermediate- and high-velocity clouds
Published in Monthly notices of the Royal Astronomical Society (21-07-2006)“…We present Ca-iiK (λair= 3933.661-Å) interstellar observations towards 20 early-type stars, to place lower distance limits to intermediate- and high-velocity…”
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15
Early-type stars in the Galactic halo from the Palomar–Green survey – III. Completion of a magnitude range limited sample
Published in Monthly notices of the Royal Astronomical Society (11-04-2004)“…High-resolution (R≈ 40 000) echelle spectroscopic observations of 13 high-latitude early-type stars are presented. These stars comprise the final part of a…”
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Observations towards early-type stars in the ESO-POP Survey – II. Searches for intermediate- and high-velocity clouds
Published in Monthly notices of the Royal Astronomical Society (01-07-2007)“…We present Ca ii K and Ti ii optical spectra of early-type stars taken mainly from the ultraviolet and visual echelle spectrograph (UVES) Paranal Observatory…”
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17
A non-LTE abundance analysis of the post-AGB star ROA 5701
Published in Monthly notices of the Royal Astronomical Society (01-06-2006)“…An analysis of high-resolution Anglo-Australian Telescope (AAT)/University College London Échelle Spectrograph (UCLÉS) optical spectra for the ultraviolet…”
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18
High-resolution spectroscopic observations of post-asymptotic giant branch candidates from the Edinburgh—Cape Survey
Published in Monthly notices of the Royal Astronomical Society (01-11-2005)“…High spectral resolution (R∼ 40 000) and signal-to-noise optical spectra, obtained at the Very Large Telescope (VLT), are presented for three post—asymptotic…”
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High-resolution spectroscopic observations of B-type stars from the Edinburgh-Cape Survey - III. Completion of a magnitude range limited survey
Published in Monthly notices of the Royal Astronomical Society (01-09-2004)“…ABSTRACT High spectral resolution (R∼ 40 000) and signal‐to‐noise ratio observations of five high Galactic latitude early‐type stars taken from the…”
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High-resolution Keck I spectroscopy of Galactic halo post-asymptotic giant branch stars
Published in Monthly notices of the Royal Astronomical Society (11-12-2002)“…Absolute and differential abundance analyses have been performed from high-resolution, high signal-to-noise ratio optical (Keck I) spectra for three evolved…”
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