Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..128..331d&link_type=abstract
Astronomy and Astrophysics Supplement, v.128, p.331-348
Astronomy and Astrophysics
Astrophysics
10
Surveys, Stars: Neutron, White Dwarfs, X-Rays: Stars, Radio Continuum: Stars
Scientific paper
This is the first in a series of three papers aiming to put strong observational constraints on the number of old accreting neutron stars in the Galaxy. Old neutron stars have been predicted to be visible as soft X-ray sources. The brightest sources are expected where the density of the interstellar medium is high. I present an X-ray survey of a complete sample of molecular clouds at high galactic latitudes based on the ROSAT All-Sky Survey. I detect 89 sources inside the projected contours of the molecular clouds and report on a comprehensive identification program. For all sources I searched astronomical catalogs and created finding charts. I also observed all sources at radio frequencies, most of them at 1.4GHz and at 8GHz. For sources with bright counterparts, optical spectra are presented. For fainter sources, optical CCD images are shown. Of all sources, 54 are securely identified and for the majority of the remaining sources likely identifications are given. I find no candidate for an old accreting neutron star in this sample. From this survey I derive an upper limit to the neutron star density of 50sr(-1) at a ROSAT count rate of 0.012s(-1) . Fig.\,9 and Fig.\,10 are only and Table\,2 is additionally available in electronic form at the CDS via http://cdsweb.u-strasbg.fr/Abstract.html
No associations
LandOfFree
Searching for old neutron stars with ROSAT. I. Soft X-ray sources in molecular clouds at high galactic latitude 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 Searching for old neutron stars with ROSAT. I. Soft X-ray sources in molecular clouds at high galactic latitude, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Searching for old neutron stars with ROSAT. I. Soft X-ray sources in molecular clouds at high galactic latitude will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1655906