Results 31 to 40 of about 412,693 (262)
THE FATE OF STELLAR MASS LOSS IN CENTRAL CLUSTER GALAXIES [PDF]
, 2011 Star formation within the central galaxies of galaxy clusters is often interpreted as being fueled by cooling of the hot intracluster medium. However, the star-forming gas is dusty, and Spitzer spectra show that the dust properties are similar to those ...
G. Mark Voit, Megan Donahue
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The Astrophysical Journal, 2023 Eta Carinae ( η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components. Over many decades, the spectrum has changed—there has been an increase in observed continuum fluxes and a decrease in Fe ii and H i emission-line ...
Augusto Damineli +25 more
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Solid Particles and Stellar Mass Loss
The Astrophysical Journal, 1974 John D. Fix, David R. Alexander
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The Astrophysical Journal, 2023 Stellar coronal mass ejections (CMEs) have recently received much attention for their impacts on exoplanets and stellar evolution. Detecting prominence eruptions, the initial phase of CMEs, as the blueshifted excess component of Balmer lines is a ...
Shun Inoue +7 more
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On stellar mass loss from galaxies in groups and clusters [PDF]
, 2017 We estimate the stellar mass that satellite galaxies lose once they enter groups (and clusters) by identifying groups in a high-resolution cosmological N-body simulation, assigning entry masses to satellite galaxies with halo abundance matching at the ...
'Edouard Tollet +4 more
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On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium [PDF]
, 2017 We quantify the gas-phase abundance of deuterium and fractional contribution of stellar mass loss to the gas in cosmological zoom-in simulations from the Feedback In Realistic Environments project.
F. Voort +7 more
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Mass loss in 2D rotating stellar models [PDF]
Proceedings of the International Astronomical Union, 2010 AbstractRadiatively driven mass loss is an important factor in the evolution of massive stars. The mass loss rates depend on a number of stellar parameters, including the effective temperature and luminosity. Massive stars are also often rapidly rotating, which affects their structure and evolution.
Lovekin, Catherine, Deupree, Robert G.
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A GRID OF MHD MODELS FOR STELLAR MASS LOSS AND SPIN-DOWN RATES OF SOLAR ANALOGS [PDF]
, 2013 Stellar winds are believed to be the dominant factor in the spin-down of stars over time. However, stellar winds of solar analogs are poorly constrained due to observational challenges.
O. Cohen, J. Drake
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Photoevaporation versus core-powered mass-loss: model comparison with the 3D radius gap [PDF]
Monthly notices of the Royal Astronomical Society, 2021 The EUV/X-ray photoevaporation and core-powered mass-loss models are both capable of reproducing the bimodality in the sizes of small, close-in exoplanets observed by the Kepler space mission, often referred to as the ‘radius gap’.
James G. Rogers +3 more
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Effects of Stellar Mass Loss on the Formation of Planetary Nebulae [PDF]
, 1983 Sun Kwok
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