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Hypergiant
Supernova 2007Bi Was a Pair-Instability Explosion
Astrophysics VLT/UVES Spectroscopy of Wray 977, the Hypergiant
Astronomy General Information
The Yellow Hypergiant HR 5171 A: Resolving a Massive Interacting Binary in the Common Envelope Phase,
The Yellow Hypergiants HR 8752 and Ρ Cassiopeiae Near the Evolutionary Border of Instability1
Blue Supergiants As Descendants of Magnetic Main Sequence Stars
X-Ray Searches for Axions from Super Star Clusters Christopher Dessert, Joshua W
Luminous and Variable Stars in M31 and M33. III. the Yellow and Red Supergiants and Post-Red Supergiant Evolution
On the Evolution and Fate of Super-Massive Stars
A Hypergiant with Pulsar Companion
Stsci Newsletter: 2017 Volume 034 Issue 02
On the Evolution and Fate of Super-Massive Stars
Massive Stars: Life and Death
The Herschel View of the Nebula Around the Luminous Blue Variable Star AG Carinae,,
Two Decades of Hypergiant Research
Radiative Transfer in Stellar Atmospheres
Stellar Winds and Hydrodynamic Atmospheres of Stars
An Astrophysical Laboratory: Understanding and Exploiting the Young Massive Cluster Westerlund 1
Top View
The Hypergiant HR 8752 Evolving Through the Yellow Evolutionary Void,
The Most Massive Stars Known 22
A VLT/FLAMES Survey for Massive Binaries in Westerlund 1 IV
Highest-Energy Supernovae Might Look Quite Spectacular from a Planet
VLT/UVES Spectroscopy of Wray 977, the Hypergiant Companion to the X-Ray Pulsar GX301−2
The Formation of Black-Holes in Low-Mass X-Ray Binaries Simon F
2018 Div. C (High School) Astronomy Help Session Sunday, Feb. 18Th, 2018 Stellar Evolution and Type II Supernovae Scott Jackson Mt
Super Supernovae
Driebe Et Al.: Probing the Brgamma-Emitting Wind Region
Where Do Lbvs Come From? …And Where Do WR Stars Come From?
Red Supergiants, Yellow Hypergiants, and Post-RSG Evolution
New ESO Publications the LOCAL GROUP: EUROPEAN SL
Arxiv:2008.03305V2 [Hep-Ph] 1 Mar 2021
INTEGRAL View of Tev Sources: a Legacy for the CTA Project
Luminous Blue Variables – Characteristics and Definition
AS 314: a Dusty A–Type Hypergiant By
Two Decades of Hypergiant Research
The Mass-Loss History of the Red Hypergiant VY Cma*