Binary interaction dominates the evolution of massive stars. - Wikidata - awgldk - TriplyDB

Binary interaction dominates the evolution of massive stars.

Binary interaction dominates the evolution of massive stars.

http://www.wikidata.org/entity/Q34290605

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Fundamental properties of nearby single early B-type stars The VLT-FLAMES Tarantula Survey Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death Eclipsing high-mass binaries. I. Light curves and system parameters for CPD -51{deg}8946, PISMIS 24-1, and HD 319702 The Evolution of Compact Binary Star Systems.Formation of the first three gravitational-wave observations through isolated binary evolution The evolution of massive stars: bridging the gap in the Local Group.Gamma-Ray Burst Progenitors The dynamical importance of binary systems in young massive star clusters The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase The evolution of massive stars and their spectra. I. A non-rotating 60 M_{sun}_ star from the zero-age main sequence to the pre-supernova stage The Wolf-Rayet stars in the Large Magellanic Cloud The Red Supergiant Content of the Local Group Wolf-Rayet stars in the Small Magellanic Cloud Ejection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C.Massive stars on the verge of exploding: the properties of oxygen sequence Wolf-Rayet stars The death of massive stars - II. Observational constraints on the progenitors of Type Ibc supernovae On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613 Red supergiants and stellar evolution MY Camelopardalis, a very massive merger progenitor 450 d of Type II SN 2013ej in optical and near-infrared Evidence of quasi-chemically homogeneous evolution of massive stars up to solar metallicity Hypervelocity runaways from the Large Magellanic Cloud The evolution of rotating very massive stars with LMC composition Luminous blue variables: An imaging perspective on their binarity and near environment The binary merger channel for the progenitor of the fastest rotating O-type star VFTS 102 Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen Binary companions of nearby supernova remnants found with Gaia High-mass X-ray binaries in the Milky Way Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh Effects of binary stellar populations on direct collapse black hole formation Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction Supernova remnants in the Local Group – I. A model for the radio luminosity function and visibility times of supernova remnants Nearby supernova host galaxies from the CALIFA survey A comprehensive comparative test of seven widely used spectral synthesis models against multi-band photometry of young massive-star clusters Hubble Tarantula Treasury Project – IV. The extinction law The blue supergiant MN18 and its bipolar circumstellar nebula Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources Near-infrared spectroscopy of 20 newChandrasources in the Norma arm Discovery of a magnetic field in the rapidly rotating O-type secondary of the colliding-wind binary HD 47129 (Plaskett's star)

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Binary interaction dominates the evolution of massive stars.

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2012 nî lūn-bûn

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2012 թուականի Յուլիսին հրատարակուած գիտական յօդուած

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2012 թվականի հուլիսին հրատարակված գիտական հոդված

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2012年の論文

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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Binary interaction dominates the evolution of massive stars.

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