Meet the AAS Keynote Speakers: Lars Bildsten
Professor Lars Bildsten understand the values of change — stellar change, that is. Read more about his research and career before his keynote at #AAS231!
Professor Lars Bildsten understand the values of change — stellar change, that is. Read more about his research and career before his keynote at #AAS231!
NGC 3199 is only the fourth Wolf-Rayet nebula to be observed in X-rays. Toala et al. present chemical abundances for this nebula and find that the star that produces it, once considered a runaway star, might not be so far from home after all.
The authors of today’s paper take us on a treasure hunt of baby massive stars, come join us!
Ever wondered what baby massive stars look like? Let’s find out!
Many massive stars die as supernovae, although connection between a star’s life and it’s death is unclear. Today’s paper uses statistical distributions of massive stars and supernovae to link together both ends of the story.
Are more massive stars more likely to have planets? Read on to find out…