Works matching IS 17439213 AND DT 2024 AND VI 18 AND IP S361
Results: 123
IAU volume 18 issue 361 Cover and Back matter.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. b1, doi. 10.1017/S1743921324000395
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CMD for atmospheres of massive stars created by using CMFGEN synthetic spectra.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 179, doi. 10.1017/S1743921323004404
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Observations south of HD 5980.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 334, doi. 10.1017/S1743921323003976
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Massive Stars in Low-metallicity Galaxies in the CLASSY Survey.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 26, doi. 10.1017/S1743921323001771
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Double Vision: Combining X-ray and Spectropolarimetric Observations of WR Binaries.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 502, doi. 10.1017/S1743921322005014
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How to make an 85 Solar Mass Black Hole.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 391, doi. 10.1017/S1743921322003441
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Stellar Atmospheres and Supernovae: Systematic Errors.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 127, doi. 10.1017/S174392132200343X
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Ultraviolet observations of massive stars and the instrumentation to come.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 621, doi. 10.1017/S1743921322003416
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X-raying massive stars and their feedback near and far.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 479, doi. 10.1017/S1743921322003404
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The Gaia view on massive stars: EDR3 and what to expect from DR3.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 76, doi. 10.1017/S1743921322003398
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Progenitors and companions of stripped-envelope supernovae.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 612, doi. 10.1017/S1743921322003362
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Stellar Structure and Evolution of Massive Rotating Single Stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 343, doi. 10.1017/S1743921322003349
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Using machine learning to investigate the populations of dusty evolved stars in various metallicities.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 454, doi. 10.1017/S1743921322003337
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Astro+: Design, construction, and scientific exploitation of a large-scale massive star spectroscopic database.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 197, doi. 10.1017/S1743921322003295
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A comprehensive empirical investigation of Galactic fast-rotating O-type stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 236, doi. 10.1017/S1743921322003283
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Upper Mass-Loss Limits and Clumping in the Intermediate and Outer Wind Regions of OB stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 194, doi. 10.1017/S1743921322003271
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The CubeSpec space mission: Asteroseismology of massive stars from time-series optical spectroscopy.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 630, doi. 10.1017/S174392132200326X
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Fundamental parameters for 222 B-type stars for the X-shooter Spectral Library.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 108, doi. 10.1017/S1743921322003258
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Properties of Primitive Galaxies.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 485, doi. 10.1017/S1743921322003246
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Evolution and final fate of massive post-common-envelope binaries.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 339, doi. 10.1017/S1743921322003222
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Red Supergiants in M31: The Humphreys-Davidson limit at high metallicity.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 422, doi. 10.1017/S1743921322003210
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Exploring a direct observational method to measure high-redshift cloud collapse timescales and GRB progenitor lifetimes.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 584, doi. 10.1017/S1743921322003209
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The evolution of binary-stripped stars: consequences for supernovae and black hole formation.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 596, doi. 10.1017/S1743921322003192
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The Nature of Unseen Companions in Massive Single-Line Spectroscopic Binaries.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 267, doi. 10.1017/S1743921322003180
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A SITELLE view of the Galactic Wolf-Rayet Nebulae NGC6888 and NGC2359.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 515, doi. 10.1017/S1743921322003179
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Polstar : a FUV Spectropolarimetry Mission.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 633, doi. 10.1017/S1743921322003167
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ASSESSing evolved massive stars in NGC 6822 and IC 10.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 432, doi. 10.1017/S1743921322003155
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Stability analysis of radial oscillation modes in massive stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 251, doi. 10.1017/S1743921322003143
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A search for correlations between Wolf-Rayet stochastic wind variability and stellar parameters.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 507, doi. 10.1017/S1743921322003131
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Observations of Very Low-Metallicity Massive Stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 36, doi. 10.1017/S174392132200312X
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Dependence of Wolf-Rayet wind clumping on the surface temperature.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 493, doi. 10.1017/S1743921322003118
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Luminous red supergiants in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 429, doi. 10.1017/S1743921322003106
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Open questions in massive star research.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 1, doi. 10.1017/S1743921322003088
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Nitrogen production in population III stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 259, doi. 10.1017/S1743921322003076
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Hunting for red supergiant binaries: UVIT photometry of the SMC.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 279, doi. 10.1017/S1743921322003064
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Infrared studies of the massive stellar population at the Galactic Center and the inner disk.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 114, doi. 10.1017/S1743921322003052
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Strong lithium lines in red supergiants at different metallicities.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 410, doi. 10.1017/S1743921322003040
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Constraining physical processes in pre-supernovae massive star evolution.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 224, doi. 10.1017/S1743921322003039
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Wolf-Rayet stars: recent advances and persisting problems.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 465, doi. 10.1017/S1743921322003015
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Deciphering hard disks.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 319, doi. 10.1017/S1743921322003003
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Formation of Very Low-metallicity Stars.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 521, doi. 10.1017/S1743921322002988
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MWC 656: A Be+BH or a Be+sdO?
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 332, doi. 10.1017/S1743921322002976
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Metallicity distributions of core-collapse supernovae within 30Mpc: Evidence for a lack of single massive Ib progenitors at low metallicities.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 590, doi. 10.1017/S1743921322002964
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Constraints on the stellar upper mass limit from simulations of UV disk ablation.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 550, doi. 10.1017/S1743921322002952
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M 1-67 and RCW 58: nebulae around WN8h stars formed through CE evolution.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 499, doi. 10.1017/S1743921322002927
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Study of the Be/X-ray binary IGR J21343+4738 physical parameters based on the 15-years monitoring.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 321, doi. 10.1017/S1743921322002915
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Formation of black holes in the pair-instability mass gap: Hydrodynamical simulation of a massive star collision & evolution of a post-collision star.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 302, doi. 10.1017/S1743921322002903
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Numerical modeling of IR SEDs of dusty CCSN within a Bayesian framework.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 615, doi. 10.1017/S1743921322002897
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Two-dimensional models of fast rotating stars and mixing processes.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 359, doi. 10.1017/S1743921322002885
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Wind line variability and intrinsic errors in observational mass loss rates.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 205, doi. 10.1017/S174392132200285X
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