A thick-disc origin for Tycho Brahe's 1572 supernova?

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10

Stars: Individual: Tycho G, Supernovae: Individual: Sn 1572

Scientific paper

The very recent suggestion for the identification of a faint G-type subgiant, dubbed `Tycho G', as the binary progenitor of Tycho Brahe's 1572 Type Ia supernova by Ruiz-Lapuente et al. is essentially based on the peculiar space velocity of the star. Here we demonstrate that the kinematics of Tycho G are likewise in keeping with the stars of the Milky Way's thick-disc population. Hence we may well be seeing an object that is only coincidentally passing in the vicinity of the supernova remnant, or Tycho Brahe and his contemporaries may indeed have witnessed the late explosion of one of the first stars in the Galaxy.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

A thick-disc origin for Tycho Brahe's 1572 supernova? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A thick-disc origin for Tycho Brahe's 1572 supernova?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A thick-disc origin for Tycho Brahe's 1572 supernova? will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1599760

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.