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- Teacherguide Starevolution8
- B-Type Main-Sequence Star
- The Metallicity Evolution of Star-Forming Galaxies from Redshift 0 to 3: Combining Magnitude Limited Survey with Gravitational Lensing T.-T
- Post Main Sequence Evolution
- PAIR-INSTABILITY SUPERNOVAE (Rakavy, Shaviv, and Zinamon (1967); Barkat, Rakavy and Sack (1967))
- The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
- EXPLAINING the MORPHOLOGY of SUPERNOVA REMNANT (SNR) 1987A with the JITTERING JETS EXPLOSION MECHANISM Ealeal Bear1 and Noam Soker1,2 Draft Version April 27, 2018
- Properties of Stars
- Physical Parameters of Open Clusters with Gaia DR2
- Astronomy 10
- Download This Article in PDF Format
- Lecture 8 Overshoot Mixing, Semiconvection, Mass Loss, and Rotation
- Stellar Evolution
- Stars: Introduction
- Stellar Populations in the Large Magellanic Cloud: Evidence for A
- How Big Are Stars? How Do We Know?
- Stellar Evolution Gets Even More Complicated When the Crescent Nebula Pair- Type Ii Instability Star Has a Nearby Companion
- Stellar Associations: a Variable Stars Nurser
- Exam #2 Review
- Unit 03, the Stars
- Bumpy Light Curves of Interacting Supernovae
- Measuring Distances and Reddenings for a Billion Stars: Towards a 3D
- Astronomy Science Class – Part 1
- Pair Instability Supernovae: Light Curves and Spectra Daniel Kasen Stan Woosley, Alex Heger H H He He Si/Mg
- Crab Nebula: Pulsar During a Supernova, the Core of a Massive
- Absolute Brightness: the Apparent Brightness a Star Would Have If It Were Placed at a Standard Distance of 10 Parsecs from Earth