Astronomers have identified six massive stars before they exploded as core-collapse supernovae

A team led by Caltech's recently made some very interesting finds in the Hubble archives, where they observed the sites of six supernovae to learn more about their stars. Their observations were part of the Hubble Space Telescope Snapshot program, where astronomers use HST images to chart the life cycle and evolution of stars, galaxies, and other celestial objects. From this, they were able to place constraints on the size, mass, and other key characteristics of the progenitor stars and what they experienced before experiencing core collapse.

The team was led by Dr. Schuyler D. Van Dyk, a senior research scientist with Caltech's Infrared Processing and Analysis Center (IPAC). His teammates included researchers from the University of California, Berkeley, the Space Telescope Science Institute, the University of Arizona's Steward Observatory, the University of Hawai'i's Institute for Astronomy, and the School of Physics and Astronomy at the University of Minnesota. Their findings were published in a paper titled "The disappearance of six supernova progenitors" that will appear in the Monthly Notices of the Royal Astronomical Society.

The Hubble Ultra Deep Field seen in ultraviolet, visible, and infrared light. Credit: NASA, ESA, H. Teplitz and M. Rafelski (IPAC/Caltech), A. Koekemoer (STScI), R. Windhorst (Arizona State University), and Z. Levay (STScI)

The Whirlpool galaxy (spiral galaxy M51, NGC 5194), a classic spiral galaxy located in the Canes Venatici constellation, and its companion NGC 5195. Credit: NASA/ESA

Artist’s impression of a supernova remnant. Credit: ESA/Hubble