Results 161 to 170 of about 11,425 (209)

Interaction of SN Ib 2004dk with a Previously Expelled Envelope. [PDF]

Astrophys J, 2019
Pooley D, Wheeler JC, Vinkó J, Dwarkadas VV, Szalai T, Silverman JM, Griesel M, McCullough M, Marion GH, MacQueen P.   +9 more
europepmc   +1 more source

A rotating fast bipolar wind and disk system around the B[e]-type star MWC 922. [PDF]

Astron Astrophys, 2019
Sánchez Contreras C, Báez-Rubio A, Alcolea J, Castro-Carrizo A, Bujarrabal V, Martín-Pintado J, Tafoya D.   +6 more
europepmc   +1 more source

Retrograde Accretion Disks in High-Mass Be/X-ray Binaries. [PDF]

Mon Not R Astron Soc Lett, 2017
Christodoulou DM, Laycock SGT, Kazanas D.   +2 more
europepmc   +1 more source

Predicting the nature of supernova progenitors. [PDF]

Philos Trans A Math Phys Eng Sci, 2017
Groh JH.
europepmc   +1 more source

Strong Gravitational Lensing and Microlensing of Supernovae. [PDF]

Space Sci Rev
Suyu SH, Goobar A, Collett T, More A, Vernardos G.   +4 more
europepmc   +1 more source

ALMA Compact Array observations of the Fried Egg nebula: Evidence for large-scale asymmetric mass-loss from the yellow hypergiant IRAS 17163-3907. [PDF]

Astron Astrophys, 2017
Wallström SH, Lagadec E, Muller S, Black JH, Cox NL, Galván-Madrid R, Justtanont K, Longmore S, Olofsson H, Oudmaijer RD, Quintana-Lacaci G, Szczerba R, Vlemmings W, van Winckel H, Zijlstra A.   +14 more
europepmc   +1 more source

NEW YOUNG STARS AND BROWN DWARFS IN THE UPPER SCORPIUS ASSOCIATION. [PDF]

Astron J, 2018
Luhman KL, Herrmann KA, Mamajek EE, Esplin TL, Pecaut MJ.   +4 more
europepmc   +1 more source

Triggered Star Formation inside the Shell of a Wolf-Rayet Bubble as the Origin of the Solar System. [PDF]

Astrophys J, 2017
Dwarkadas VV, Dauphas N, Meyer B, Boyajian P, Bojazi M.   +4 more
europepmc   +1 more source

Near-infrarred spectro-interferometry of red giant and supergiant stars

, 2015
Las estrellas supergigantes rojas son estrellas frías y muy masivas que se encuentran en la fase previa a las estrellas Wolf-Rayet y a las supernovas. Presentan extensas atmósferas y fuertes vientos estelares que dan lugar a una importante pérdida de masa.
openaire   +1 more source

Excavating the Explosion and Progenitor Properties of Type IIP Supernovae via Modeling of their Optical Light Curves. [PDF]

Astrophys J, 2019
Ricks W, Dwarkadas VV.
europepmc   +1 more source