Luminous blue variable
![Arxiv:1912.00994V2 [Astro-Ph.SR] 4 Sep 2020 Which Can Be Observed with Electromagnetic Radiation Metallicity (E.G](https://docslib.b-cdn.net/cover/2806/arxiv-1912-00994v2-astro-ph-sr-4-sep-2020-which-can-be-observed-with-electromagnetic-radiation-metallicity-e-g-4542806.webp)
Top View
- Radio Detection of Nebulae Around Four Luminous Blue Variable Stars in the Large Magellanic Cloud
- Blue Supergiant Star
- The Molecular Gas Around the Luminous Blue Variable Star G24.73+0.69
- A VLT/FLAMES Survey for Massive Binaries in Westerlund 1 IV
- Spectroscopy and Interferometry of the Winds of Luminous Blue Variables
- Progenitors of Core-Collapse Supernovae
- Astronomy Div C 2014 Help Session V0
- Stars with Special Characteristics
- 2018 Div. C (High School) Astronomy Help Session Sunday, Feb. 18Th, 2018 Stellar Evolution and Type II Supernovae Scott Jackson Mt
- Cygnus X-1 Contains a 21-Solar Mass Black Hole – Implications for Massive Star Winds
- Life Cycle of High Mass Stars Supernovae Neutron Stars, Pulsars, Pulsar Wind Nebulae, Magnetars Quark-Nova Stars Gamma-Ray Bursts (Grbs)
- IAU Symposium 250 Massive Stars As Cosmic Engines
- Mid-Infrared VISIR and Spitzer Observations of the Surroundings of the Magnetar SGR 1806-20
- CLOSE BINARY MODELS for LUMINOUS BLUE VARIABLE STARS J. S. GALLAGHER Lowell Observatory 1400 West Mars Hill Road Flagstaff, Ariz
- Core Collapse Supernovae Our Topic Today Is the Post-Main Sequence
- SN 2015Bh: NGC 2770'S 4Th Supernova Or a Luminous Blue
- A Giant Outburst Two Years Before the Core- Collapse of a Massive Star