Results 231 to 240 of about 801 (259)

Water Versus Land on Temperate Rocky Planets. [PDF]

Space Sci Rev
Guimond CM, Spohn T, Berdyugina S, Byrne PK, Coltice N, Glaser DM, Lingam M, Lineweaver CH, Cawood PA.   +8 more
europepmc   +1 more source

Chip-integrated spectroscopy capable of temperature retrieval. [PDF]

Sci Rep
Du Y, Sua YM, Kumar S, Zhang J, Li X, Hu Y, Ghuman P, Huang Y.   +7 more
europepmc   +1 more source

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

Some of the next articles are maybe not open access.

Related searches:

Accretion disk dynamics, photoionized plasmas, and stellar opacities

Physics of Plasmas, 2009
We present a brief review on the atomic kinetics, modeling and interpretation of astrophysical observations, and laboratory astrophysics experiments. The emphasis is on benchmarking of opacity calculations relevant for solar structure models, photoionized plasmas research, the magnetohydrodynamic numerical simulation of accretion disk dynamics, and a ...
Roberto C Mancini, Bailey J E, Mancini R C   +2 more
exaly   +3 more sources

The development of large-scale instability in Keplerian stellar accretion disks

Astronomy Reports, 2012
Our previous studies of large-scale vortical flows arising in shear flows of stellar accretion disks with Keplerian azimuthal velocity distributions as a result of the development of small perturbations are continued. The development of large-scale instability in an accretion disk is investigated via mathematical modeling.
V M Chechetkin, Chechetkin V M
exaly   +2 more sources

Formation and Evolution of Minerals in Accretion Disks and Stellar Outflows

Lecture Notes in Physics, 2003
The contribution discusses dust formation and dust processing in oxygen rich stellar outflows under non-explosive conditions, and in circumstellar discs. The main topics are calculation of solid-gas chemical equilibria, the basic concepts for calculating dust growth under non-equilibrium conditions, dust processing by annealing and solid diffusion, a ...
exaly   +2 more sources

Accretion disks in stellar X-ray sources

Space Science Reviews, 1982
Verbunt Frank
exaly   +2 more sources

Accretion Disks in Compact Stellar Systems

1993
Disk instabilities in stellar accretion disks, J. Cannizzo and F. Meyer angular momentum transport in low mass accretion disks, E.T. Vishniac emission lines from accretion disks, E.L. Robinson eclipse mapping of accretion disks, K. Horne disk atmospheres, G. Shaviv discs and magnetospheres, A. King winds and boundary layers in accretion disks, J.
openaire   +2 more sources

Alfvén Waves in Dusty Proto-Stellar Accretion Disks

2012
The magneto-rotational instability (MRI) is believed to be the mechanism responsible for a magneto-hydrodynamic (MHD) turbulence that could lead to the accretion observed in proto-stellar accretion disks. A minimum amount of ionization in this medium is necessary for the MRI to take place.
Aline de Almeida Vidotto, Vera Jatenco-Pereira   +1 more
openaire   +1 more source