- We will determine the parallax, using the HST (approved cycle 7 time),
hopefully in April and October 1998.
- The HST observations will also yield the proper motion. If this points
back to an identifiable OB association, it will yield the age.
- We are generating improved atmospheric models (see
- With the model atmospheres and a distance, we intend to determine the
radius of this neutron star.
Return to top of poster
To previous page
To next page