Results 91 to 100 of about 77,155 (253)
Dust in the Magellanic Clouds [PDF]
Symposium - International Astronomical Union, 1991 The dust content of the Magellanic Clouds can be studied using optical, ultraviolet, infrared and, indirectly, radio wavelength data. All recent studies show that the dust content is lower than that of the Milky Way Galaxy for both Clouds and that the optical properties of the dust are different.
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Be Stars in the Magellanic Clouds [PDF]
International Astronomical Union Colloquium, 2000 AbstractWe present the results of our studies of Be stars within the Magellanic Clouds. We have studied the Be population within four young populous clusters, NGC 330 in the SMC, NGC 1818, 2004 and 2100 in the LMC as well as the field population around NGC 2004.
Stefan C. Keller +2 more
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The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
UniverseSimulations of structure formation in the standard cold dark matter cosmological model quantify the dark matter halos of galaxies. Taking into account dynamical friction between dark matter halos, we investigate the past orbital dynamical evolution of ...
Wolfgang Oehm, Pavel Kroupa
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The Astrophysical Journal, 2023 We present the first compelling evidence of shock-heated molecular clouds associated with the supernova remnant (SNR) N49 in the Large Magellanic Cloud (LMC).
H. Sano +30 more
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The Chemical Enrichment History of the Magellanic Clouds Field Populations [PDF]
, 2008 We report the results of our project devoted to study the chemical enrichment history of the field population in the Magellanic Clouds using Ca II triplet spectroscopy.
arxiv +1 more source
Evolution and the period-luminosity relation for red supergiants in the Magellanic Clouds [PDF]
, 2013 Excitation of radial pulsations in red supergiants of Magellanic Clouds is investigated using the stellar evolution calculations and the self-consistent solution of the equations of radiation hydrodynamics and turbulent convection. The stars with initial
Fadeyev, Yuri A.
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The Astrophysical Journal, 2023 GRB 230307A is the second brightest gamma-ray burst detected in more than 50 years of observations and is located in the direction of the Magellanic Bridge. Despite its long duration, it is most likely the result of the merger of a compact binary ejected
Sandro Mereghetti +4 more
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Effects of Metallicity on the Rotation Rates of Massive Stars
, 2004 Recent theoretical predictions for low metallicity massive stars predict that these stars should have drastically reduced equatorial winds (mass loss) while on the main sequence, and as such should retain most of their angular momentum.
Amanda J. Sprague +7 more
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Radio pulsars in the Magellanic Clouds [PDF]
Symposium - International Astronomical Union, 1991 The Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) have been searched for radio pulsars using the 64-m Parkes radiotelescope. The search has resulted in the discovery of four pulsars. Observed dispersion measures to each suggest that three lie in the Clouds (two in the LMC, one in the SMC) and that the fourth, which was found in the ...
David McConnell +6 more
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Toward a Complete Understanding of the Magellanic Stream Formation [PDF]
, 2019 The Magellanic Clouds have lost most of their gas during their passage by the Milky Way, a property that has never been successfully modeled. Here we use accurate and mesh-free hydrodynamic simulations to reproduce the Magellanic Stream and the Magellanic Clouds in the frame of a 'ram-pressure plus collision' model.
arxiv +1 more source