Results 181 to 190 of about 11,425 (209)

Gamma-ray bursts and their use as cosmic probes. [PDF]

R Soc Open Sci, 2017
Schady P.
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Young Stellar Objects in the Massive Star-forming Regions W51 and W43. [PDF]

Astrophys J, 2017
Saral G, Hora JL, Audard M, Koenig XP, Martínez-Galarza JR, Motte F, Nguyen-Luong Q, Saygac AT, Smith HA.   +8 more
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Building Blocks of Dust: A Coordinated Laboratory and Astronomical Study of AGB Stars. [PDF]

J Mol Spectrosc, 2019
McCarthy MC, Gottlieb CA, Cernicharo J.
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Through the magnifying glass: ALMA acute viewing of the intricate nebular architecture of OH231.8+4.2. [PDF]

Astron Astrophys, 2018
Sánchez Contreras C, Alcolea J, Bujarrabal V, Castro-Carrizo A, Prieto LV, Santander-García M, Quintana-Lacaci G, Cernicharo J.   +7 more
europepmc   +1 more source

The exceptional X-ray evolution of SN 1996cr in high resolution. [PDF]

Mon Not R Astron Soc, 2019
Quirola-Vásquez J, Bauer FE, Dwarkadas VV, Badenes C, Brandt WN, Nymark T, Walton D.   +6 more
europepmc   +1 more source

Directed gas phase formation of silicon dioxide and implications for the formation of interstellar silicates. [PDF]

Nat Commun, 2018
Yang T, Thomas AM, Dangi BB, Kaiser RI, Mebel AM, Millar TJ.   +5 more
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Interpreting signals from astrophysical transient experiments. [PDF]

Philos Trans A Math Phys Eng Sci, 2013
O'Brien PT, Smartt SJ.
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Pulsating red giant and supergiant stars in the Local Group dwarf galaxy Andromeda I

Iranian Journal of Astronomy and Astrophysics, 2017
Elham Saremi, Abbas Abedi, Atefeh Javadi, Jacco van Loon , Habib Khosroshahi   +4 more
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Atmosphere tomography of red supergiant stars

EAS Publications Series, 2013
3-D simulations suggest that the atmospheres of red super-giants are subject to large-amplitude convective motions, which are suspected to generate supersonic motions and shocks. We perform tomography of supergiant-star atmospheres, on temporal series of high-resolution spectra and on 3-D hydrodynamical synthetic spectra.
S. Lion, S. Van Eck, A. Chiavassa, B. Plez, A. Jorissen   +4 more
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Global radiation-hydrodynamics simulations of red supergiant stars

EAS Publications Series, 2013
The small-scale surface granulation on cool main-sequence stars and white dwarfs influences the overall appearance of these objects only weakly. And it is only indirectly observable by analyzing e.g. line-shapes or temporal fluctuations – except for the Sun.
B. Freytag, A. Chiavassa
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