Supernovas decrease the mass of a star substantially
The remnant is much more dense however which increases the strength of the gravitational field at the new surface
In the case of black holes I'd guess that the event horizon has a smaller radius than the original star prior to its giant phase
Finally if you draw a large enough circle around the remnant and surrounding nebula you'll describe a system which will have a similar, but not identical, mass to the original star which would be gravitationally similar at enough of a distance.
The real discrepancy in mass will be from matter being converted to energy over the life of the star, especially during the supernova. I'm not sure what fraction of the mass this usually is
The remnant is much more dense however which increases the strength of the gravitational field at the new surface
In the case of black holes I'd guess that the event horizon has a smaller radius than the original star prior to its giant phase
Finally if you draw a large enough circle around the remnant and surrounding nebula you'll describe a system which will have a similar, but not identical, mass to the original star which would be gravitationally similar at enough of a distance.
The real discrepancy in mass will be from matter being converted to energy over the life of the star, especially during the supernova. I'm not sure what fraction of the mass this usually is
