ChaMPlane: latest results and future projects

Details ChaMPlane: latest results and future projects ChaMPlane: latest results and future projects

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.193s&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Physics

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The Chandra Multiwavelength Plane Survey (ChaMPlane) is based on Chandra deep X-ray observations close to the Galactic Plane and the Galactic Center. We obtained optical imaging data (NOAO 4m Mosaic), and are conducting a follow-up spectroscopy and near-infrared (NOAO 4m ISPI mainly) program in order to detect counterparts to the X-ray sources and identify their nature. Based on this dataset, we aim to identify peculiar Galactic populations of objects such as accreting white dwarfs, neutron stars and black holes in order to study the distribution and the evolution of those populations. We present here the latest results and the work in progress.

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