Results 281 to 290 of about 985,930 (333)

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

Fujimoto S, Ouchi M, Kohno K, Valentino F, Giménez-Arteaga C, Brammer G, Furtak L, Kohandel M, Oguri M, Pallottini A, Richard J, Zitrin A, Bauer F, Boylan-Kolchin M, Dessauges-Zavadsky M, Egami E, Finkelstein S, Ma Z, Smail I, Watson D, Hutchison T, Rigby J, Welch B, Ao Y, Bradley L, Caminha G, Caputi K, Espada D, Endsley R, Fudamoto Y, González-López J, Hatsukade B, Koekemoer A, Kokorev V, Laporte N, Lee M, Magdis G, Ono Y, Rizzo F, Shibuya T, Shimasaku K, Sun F, Toft S, Umehata H, Wang T, Yajima H.   +45 more
europepmc   +1 more source

Extended hot dust emission around the earliest massive quiescent galaxy

Ji Z, Williams C, Rieke G, Lyu J, Alberts S, Sun F, Helton J, Rieke M, Shivaei I, D'Eugenio F, Tacchella S, Robertson B, Zhu Y, Maiolino R, Bunker A, Sun Y, Willmer C.   +16 more
europepmc   +1 more source

Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback

Eckert D, Gastaldello F, Lovisari L, McGee S, Pasini T, Brienza M, Kolokythas K, O'Sullivan E, Simionescu A, Sun M, Bourne M, Chen Y, Cui W, Ettori S, Finoguenov A, Gozaliasl G, Kale R, Mernier F, Oppenheimer B, Schellenberger G, Seppi R, Tempel E.   +21 more
europepmc   +1 more source

GAIA AND PHYSICS OF STELLAR INTERIORS [PDF]

EAS Publications Series, 2002
Understanding the stellar interiors is an important issue for astrophysics, but also for fundamental physics. The physical description of the stellar material implies statistical physics as well as hydrodynamics. We give examples of unsolved physical problems and their consequences for predictions of stellar properties and evolution.
Lebreton, Yveline, Baglin, Annie
openaire   +2 more sources

Some of the next articles are maybe not open access.

Related searches:

Stellar Physics and Starburst Evolution

1998
Starbursts regions offer a very interesting opportunity to study the links between stellar and galactic evolutions. Indeed starburst triggering is often related to dynamical processes. As mentioned in F. Combes’ lectures, the most spectacular starbursts occur in tidally interacting galaxies and mergers. On the other hand, many observational features of
G. Meynet
openaire   +3 more sources

The Sun as a Guide to Stellar Physics

2019
Jean-Claude Vial, Andrew Skumanich, Oddbjørn Engvold   +2 more
openaire   +3 more sources

Stellar Physics at Dome C [PDF]

EAS Publications Series, 2005
We present a short synthetic summary of prospects for stellar astrophysics from Dome C. We conclude that a progressive strategy could be defined, giving access to a 2 m-class telescope, equipped with a highly efficient optical/infrared spectrograph/spectropolarimeter and a wide-field infrared imager, in the 2008 timeframe, then ...
openaire   +1 more source

Physics optimization of stellarators

Physics of Fluids B: Plasma Physics, 1992
The theoretical and experimental development of stellarators has removed some of the specific deficiencies of this configuration, viz., the limitations in β, the high neoclassical transport, and the low collisionless confinement of α particles. These optimized stellarators can best be realized with a modular coil system.
Friedrich E. Wagner, H. Ringler, P. Merkel, H. J. Hartfuss, V. Erckmann, W. Lotz, J. Nührenberg, R. Jaenicke, J. Sapper, E. Strumberger, U. Gasparino, Georg Kühner, L. Giannone, R. Burhenn, H. Wobig, G. Grieger, A. Weller   +16 more
openaire   +2 more sources

Physics of Stellar Convection

AIP Conference Proceedings, 2009
We review recent progress using numerical simulations as a testbed for development of a theory of stellar convection, much as envisaged by John von Newmann. Necessary features of the theory, non‐locality and fluctuations, are illustrated by computer movies.
W. David Arnett, Giuliana Giobbi, Amedeo Tornambe, Gabriella Raimondo, Marco Limongi, L. A. Antonelli, Nicola Menci, Enzo Brocato   +7 more
openaire   +2 more sources