Search Results - "Thompson, I. B."
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A distance to the Large Magellanic Cloud that is precise to one per cent
Published in Nature (London) (01-03-2019)“…In the era of precision cosmology, it is essential to determine the Hubble constant empirically with an accuracy of one per cent or better 1 . At present, the…”
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An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent
Published in Nature (London) (07-03-2013)“…Observations of eight long-period, late-type eclipsing-binary systems composed of cool, giant stars are used to determine a distance to the Large Magellanic…”
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The dynamical mass of a classical Cepheid variable star in an eclipsing binary system
Published in Nature (London) (25-11-2010)“…Cepheid variable mass Cepheid variable stars have been important in the development of modern astrophysics through their use in establishing cosmic distances,…”
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Circumstellar material in type Ia supernovae via sodium absorption features
Published in Science (American Association for the Advancement of Science) (12-08-2011)“…Type Ia supernovae are key tools for measuring distances on a cosmic scale. They are generally thought to be the thermonuclear explosion of an accreting white…”
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ASASSN-15lh: A highly super-luminous supernova
Published in Science (American Association for the Advancement of Science) (15-01-2016)“…We report the discovery of ASASSN-15lh (SN 2015L), which we interpret as the most luminous supernova yet found. At redshift z = 0.2326, ASASSN-15lh reached an…”
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Toward Early-type Eclipsing Binaries as Extragalactic Milestones. III. Physical Properties of the O-type Eclipsing Binary OGLE LMC-ECL-21568 in a Quadruple System
Published in The Astrophysical journal (01-05-2024)“…Abstract We present the results from a complex study of an eclipsing O-type binary (Aa+Ab) with the orbital period of P A = 3.2254367 days that forms part of…”
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RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system
Published in Nature (London) (05-04-2012)“…The pulsating star OGLE-BLG-RRLYR-02792 is known to be a member of an eclipsing binary system, and its mass is now determined to be only 0.26 times that of the…”
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ON THE EVOLUTIONARY AND PULSATION MASS OF CLASSICAL CEPHEIDS. III. THE CASE OF THE ECLIPSING BINARY CEPHEID CEP0227 IN THE LARGE MAGELLANIC CLOUD
Published in The Astrophysical journal (20-04-2012)“…We present a new Bayesian approach to constrain the intrinsic parameters (stellar mass and age) of the eclipsing binary system-CEP0227-in the Large Magellanic…”
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An Intermediate Luminosity Transient in NGC 300: The Eruption of a Dust-Enshrouded Massive Star
Published in The Astrophysical journal (10-07-2009)“…We present multi-epoch high-resolution optical spectroscopy, UV/radio/X-ray imaging, and archival Hubble and Spitzer observations of an intermediate luminosity…”
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A proper motion study of the globular cluster M55
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…We have derived the absolute proper motion (PM) of the globular cluster M55 using a large set of CCD images collected with the du Pont telescope between 1997…”
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Cluster AgeS Experiment (CASE): deficiency of observed dwarf novae in globular clusters
Published in Monthly notices of the Royal Astronomical Society (11-08-2008)“…We present the results of a search for dwarf novae (DNe) in globular clusters (GCs). It is based on the largest available homogeneous sample of observations,…”
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Astronomy. ASASSN-15lh: A highly super-luminous supernova
Published in Science (American Association for the Advancement of Science) (15-01-2016)“…We report the discovery of ASASSN-15lh (SN 2015L), which we interpret as the most luminous supernova yet found. At redshift z = 0.2326, ASASSN-15lh reached an…”
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Photometric study of the variable star population in the globular cluster NGC 6397
Published in Monthly notices of the Royal Astronomical Society (01-01-2006)“…We present the results of a photometric survey for variable stars in the central region of the nearby globular cluster NGC 6397. Time-series photometry was…”
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Variable stars in the field of the old open cluster Melotte 66
Published in Monthly notices of the Royal Astronomical Society (21-09-2007)“…We report the results of photometric monitoring of the Melotte 66 field in BVI filters. 10 variables were identified with nine being new discoveries. The…”
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The Cluster AgeS Experiment (CASE) – VIII. Age and distance of the Globular Cluster 47 Tuc from the analysis of two detached eclipsing binaries
Published in Monthly notices of the Royal Astronomical Society (01-03-2020)“…ABSTRACT We use photometric and spectroscopic observations of the eclipsing binary E32 in the globular cluster 47 Tuc to derive the masses, radii, and…”
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The loudest stellar heartbeat: characterizing the most extreme amplitude heartbeat star system
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…ABSTRACT We characterize the extreme heartbeat star system MACHO 80.7443.1718 in the Large Magellanic Cloud using Transiting Exoplanet Survey Satellite (TESS)…”
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The Cluster Ages Experiment (CASE) – IX. Analysis of four detached eclipsing binaries in the globular cluster NGC 3201
Published in Monthly notices of the Royal Astronomical Society (18-10-2022)“…ABSTRACT We use photometric and spectroscopic observations of four detached eclipsing binaries in the globular cluster NGC 3201 to derive masses, radii, and…”
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Cluster Ages Experiment (CASE): Detection of a dwarf nova in the globular cluster M55
Published in Monthly notices of the Royal Astronomical Society (11-05-2005)“…We report the detection of a dwarf nova (DN) in the core region of the globular cluster M55. Six outbursts were observed during eight observing seasons…”
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Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227
Published in Monthly notices of the Royal Astronomical Society (01-12-2013)“…A novel method of analysis of double-lined eclipsing binaries containing a radially pulsating star is presented. The combined pulsating-eclipsing light curve…”
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Two planets around Kapteyn's star: a cold and a temperate super-Earth orbiting the nearest halo red dwarf
Published in Monthly notices of the Royal Astronomical Society (01-09-2014)“…Exoplanets of a few Earth masses can be now detected around nearby low-mass stars using Doppler spectroscopy. In this Letter, we investigate the radial…”
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