activity
19952003
collaborators

14 papers

astro-ph2003

Is NGC 6752 Hosting a Single or a Binary Black Hole?

Monica Colpi, Michela Mapelli, Andrea Possenti

The five millisecond pulsars that inhabit NGC 6752 display locations or accelerations remarkably different with respect to all other pulsars known in globular clusters. This may re…

astro-ph2003

Spin-perpendicular kicks from evanescent binaries formed in the aftermath of rotational core-collapse and the nature of the observed bimodal distribution of pulsar peculiar velocities

Monica Colpi, Ira Wasserman

If rotating core collapse leads to the formation of a proto-neutron star binary in super-close orbit, then the lighter star, propelled toward the minimum stable mass, explodes. The…

astro-ph2002

Young compact objects in the Solar vicinity

S. B. Popov, M. E. Prokhorov, M. Colpi +2

We present Log N -- Log S distribution for close-by young isolated neutron stars. On the basis of this distribution it is shown that the seven ROSAT isolated neutron stars (if they…

astro-ph2002

Unveiling black holes ejected from globular clusters

Alessia Gualandris, Monica Colpi, Andrea Possenti

Was the black hole in XTE J1118+480 ejected from a globular cluster or kicked away from the galactic disk?

astro-ph2002

Is NGC6752 hiding a double black hole binary in its core ?

Monica Colpi, Alessia Gualandris, Andrea Possenti

NGC6752 hosts in its halo PSR J1911-5958A, a newly discovered binary millisecond pulsar which is the most distant pulsar ever known from the core of a globular cluster. Interesting…

astro-ph2002

Young close isolated compact objects

S. B. Popov, M. E. Prokhorov, M. Colpi +2

We suggest that the seven radio-quiet isolated neutron stars observed with ROSAT are young cooling objects associated to recent near-by supernova explosions which formed runaway st…