Computer Science
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006hst..prop11010s&link_type=abstract
HST Proposal ID #11010. Cycle 15
Computer Science
Scientific paper
Extragalactic low-mass X-ray binaries LMXBs can constrain galaxy histories, but we must first understand whether LMXBs present in the fields of galaxies were formed primordially in situ or dynamically in globular clusters GCs. We propose 192 ks of ACIS-S observations + 8 orbits of HST-ACS on NGC1023, one of the nearest, massive lenticular galaxies. We will detect ~120 LMXBs and ~400 stellar clusters. Our comparison of the spatial distributions of field-LMXBs, GCs, and field stars in NGC1023 will constrain the origin of field LMXBs. Our observations will also perform the most complete census of diffuse star clusters DSCs to date. By probing the connection of DSCs to LMXBs, we will also test the dynamical formation model of LMXBs in stellar clusters.
No associations
LandOfFree
Deep Chandra and Hubble Observations of NGC 1023: Testing the Origin of Low-Mass X-ray Binaries in a Lenticular Galaxy 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 Deep Chandra and Hubble Observations of NGC 1023: Testing the Origin of Low-Mass X-ray Binaries in a Lenticular Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Deep Chandra and Hubble Observations of NGC 1023: Testing the Origin of Low-Mass X-ray Binaries in a Lenticular Galaxy will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1793245