Results 301 to 310 of about 2,730,798 (330)

Extreme weather variability on hot rocky exoplanet 55 Cancri e explained by magma temperature-cloud feedback. [PDF]

Proc Natl Acad Sci U S A
Loftus K, Luo Y, Fan B, Kite ES.
europepmc   +1 more source

Evidence of star cluster migration and merger in dwarf galaxies. [PDF]

Nature
Poulain M, Smith R, Duc PA, Marleau FR, Habas R, Durrell PR, Fensch J, Lim S, Müller O, Paudel S, Sánchez-Janssen R.   +10 more
europepmc   +1 more source

Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]

Space Sci Rev
Dickers MD, Mifsud DV, Mason NJ, Fantuzzi F.   +3 more
europepmc   +1 more source

The GD-1 Stellar Stream Perturber as a Core-collapsed Self-interacting Dark Matter Halo. [PDF]

Astrophys J Lett
Zhang X, Yu HB, Yang D, Nadler EO.
europepmc   +1 more source

Photometric detection at 7.7 μm of a galaxy beyond redshift 14 with JWST/MIRI. [PDF]

Nat Astron
Helton JM, Rieke GH, Alberts S, Wu Z, Eisenstein DJ, Hainline KN, Carniani S, Ji Z, Baker WM, Bhatawdekar R, Bunker AJ, Cargile PA, Charlot S, Chevallard J, D'Eugenio F, Egami E, Johnson BD, Jones GC, Lyu J, Maiolino R, Pérez-González PG, Rieke MJ, Robertson B, Saxena A, Scholtz J, Shivaei I, Sun F, Tacchella S, Whitler L, Williams CC, Willmer CNA, Willott C, Witstok J, Zhu Y.   +33 more
europepmc   +1 more source

An Abrupt Change in the Disk Fraction of Free-Floating Planets at the Deuterium-Burning Ignition Limit

Rodrigues T, Bouy H, Raymond S, Martín E, Bertin E, Romero JO, Barrado D, Huélamo N, Tamura M, Roig NM, Galli P, Cuillandre J.   +11 more
europepmc   +1 more source

A binary merger product as the direct progenitor of a Type II-P supernova

Niu* Z, Sun* N, Zapartas* E, Souropanis D, Cui Y, Maund JR, Andrews JJ, Briel MM, Fraser M, Gossage S, Kruckow MU, Liotine C, Liu Z, Srivas PM, Teng E, Wang X, Yang Y, Liu J.   +17 more
europepmc   +1 more source

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Stellar Evolution

Stars and Space with MATLAB Apps, 2020
Dozens of different types of stars populate the Milky Way Galaxy. The most common are main-sequence dwarfs like the Sun that fuse hydrogen into helium within their cores (the core of the Sun occupies about half its mass).
J. Kaler
semanticscholar   +5 more sources

Stellar Evolution

The Structure and Evolution of Stars, 2019
Book file PDF easily for everyone and every device. You can download and read online Stellar Evolution file PDF Book only if you are registered here.
Rebecca Elliott
openaire   +2 more sources

Stellar Evolution

2004
Abstract The physical structures and properties of stars change as they age. In this chapter, we give an overview of the way stars evolve to set the context for our later discussions. The mass is by far the most important single factor determining a star’s structure and evolution.
T W Hartquist, J E Dyson, D P Ruffle
openaire   +2 more sources