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New Insights into the Evolution of Massive Stars and Their Effects on Our Understanding of Early Galaxies [PDF]
, 2022 The observable characteristics and subsequent evolution of young stellar populations is dominated by their massive stars. As our understanding of those massive stars and the factors affecting their evolution improves, so our interpretation of distant ...
J. Eldridge, E. Stanway
semanticscholar +3 more sources
Different to the core: the pre-supernova structures of massive single and binary-stripped stars [PDF]
Astronomy & Astrophysics, 2021 The majority of massive stars live in binary or multiple systems and will interact during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae.
E. Laplace +6 more
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UV Spectroscopy of Massive Stars
Galaxies, 2020 We present a review of UV observations of massive stars and their analysis. We discuss O stars, luminous blue variables, and Wolf–Rayet stars. Because of their effective temperature, the UV (912−3200 Å) provides invaluable diagnostics not available at ...
D. John Hillier
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Luminous blue variables and the fates of very massive stars. [PDF]
Philos Trans A Math Phys Eng Sci, 2017 Smith N.
europepmc +2 more sources
Strongly interacting matter exhibits deconfined behavior in massive neutron stars [PDF]
Nature Communications, 2023 Neutron-star cores contain matter at the highest densities in our Universe. This highly compressed matter may undergo a phase transition where nuclear matter melts into deconfined quark matter, liberating its constituent quarks and gluons.
Eemeli Annala +6 more
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The Evolution of Massive Binary Stars [PDF]
Annual Review of Astronomy and Astrophysics, 2023 Massive stars play a major role in the evolution of their host galaxies and serve as important probes of the distant Universe. It has been established that the majority of massive stars reside in close binaries and interact with their companion stars ...
P. Marchant, J. Bodensteiner
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The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136 [PDF]
Monthly notices of the Royal Astronomical Society, 2020 We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of the Large Magellanic Cloud. Our sample was observed with STIS aboard the Hubble Space Telescope, is complete down to about 40 M⊙, and includes seven ...
J. Bestenlehner +13 more
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№1(1) (2018), 2023 Обсуждаются результаты наблюдений массивных звезд ранних спектральных классов в ультрафиолетовом (УФ) диапазоне, начиная от наблюдений на обсерваториях Орион-1 и 2.
А.Ф. Холтыгин
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The evolution of massive binary systems [PDF]
Serbian Astronomical Journal, 2020 The evolution of massive stars in close binary systems is significantly different from single star evolution due to a series of interactions between the two stellar components.
Petrović Jelena
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Eta Carinae: The Dissipating Occulter Is an Extended Structure
The Astrophysical Journal, 2023 Previous Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph (STIS) longslit observations of Eta Carinae ( η Car) identified numerous absorption features in both the stellar spectrum, and in the adjacent nebular spectra, along our line of ...
Theodore R. Gull +13 more
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