Young close-by neutron stars: the Gould Belt vs. the Galactic disc

Details Young close-by neutron stars: the Gould Belt vs. the Galactic disc Young close-by neutron stars: the Gould Belt vs. the Galactic disc

2003-05-30

arxiv.org/abs/astro-ph/0305599v3

Astrophys.Space Sci. 299 (2005) 117-127

Astronomy and Astrophysics

Astrophysics

14 pages, 8 figures, submitted to Ap&SS, corrected some typos

Scientific paper

10.1007/s10509-005-5160-1

We present new population synthesis calculations of close young neutron stars. In comparison with our previous investigation we use a different neutron star mass spectrum and different initial spatial and velocity distributions. The results confirm that most of ROSAT dim radioquiet isolated neutron stars had their origin in the Gould Belt. Several tens of young neutron stars can be identified in future in ROSAT data at low galactic latitudes and some of them also can be EGRET unidentified sources.

Affiliated with

Also associated with

No associations

Rating

Young close-by neutron stars: the Gould Belt vs. the Galactic disc 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 Young close-by neutron stars: the Gould Belt vs. the Galactic disc, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Young close-by neutron stars: the Gould Belt vs. the Galactic disc will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-395098