massive stars
Introducing Kathryn Neugent
Kathryn Neugent is a PhD Candidate in Astronomy at the University of Washington working with Dr. Emily Levesque. She has additionally been working as a research associate with Phil Massey at Lowell Observatory for the past 10 years. Alongside Emily and Phil, Kathryn studies massive stars (stars greater than 10 solar masses) and their evolution in the Local Group Galaxies (primarily M31, M33, and the Magellanic Clouds). Her current projects include identifying and characterizing binary Red Supergiants and their B-type star companions, understanding the evolution of Yellow Supergiants as both pre-and post- Red Supergiant objects, and directly determining the masses of Wolf-Rayet + O star binary systems. As an observational astronomer she travels the world observing at telescopes such as Gemini in Hawaii and Las Campanas in Chile. While not observing she enjoys backpacking, photography, and hanging out with her boyfriend, cat and corgi in sunny Seattle. You can stalk her more at her website: kathrynneugent.com.
Introducing Jennifer Hoffman
This week features Jennifer Hoffman. Jennifer is an associate professor of Physics & Astronomy at the University of Denver. However, she is on sabbatical from DU and is currently visiting the University of Wisconsin, where she received her Ph.D. Jennifer studies evolved massive stars and supernovae, with particular interests in binary interactions and circumstellar material. She uses observational spectropolarimetry and computational modeling to discover connections between core-collapse supernova explosions and their massive progenitor stars.
Now that she has tenure, Jennifer is also reviving longstanding interests in science education, public outreach, and diversifying the STEM community. She is still a relative Twitter newbie, but suspects that it can be a powerful tool for all of these purposes (and science too!). She normally tweets at @astroprofhoff, and her website is www.grammai.org/jhoffman/.