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arxiv: 0902.4239 · v1 · submitted 2009-02-24 · 🌌 astro-ph.HE

The Very Local Universe in X-rays

A. Ptak (1) , E. Feigelson (2) , Y.-H. Chu (3) , K. Kuntz (1) , A. Zezas (4) , S. Snowden (5) , D. de Martino (6) , G. Trinchieri (7)
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G. Fabbiano (4) W. Forman (4) G. Tagliaferri (7) R. Giacconi (1) S. Murray (4) S. Allen (8) M. Bautz (9) S. Borgani (10) N. Brandt (2) S. Campana (7) M. Donahue (11) K. Flannagan (12) R. Gilli (7) C. Jones (4) N. Miller (1) G. Pareschi (7) P. Rosati (13) D. Schneider (2) P. Tozzi (10) A. Vikhlinin (4) ((1) JHU (2) PSU (3) UIUC (4) Harvard-Smithsonian CfA (5) NASA GSFC (6) INAF-Osservatorio Astronomico di Capodimonte (7) INAF-Osservatorio Astronomico di Brera (8) Stanford University (9) MIT (10) INAF-Osservatorio Astronomico di Trieste (11) MSU (12) STSci (13) ESO)
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classification 🌌 astro-ph.HE
keywords veryx-rayaddressedbandchandradiscussexceptionalgalactic
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While the exceptional sensitivity of Chandra and XMM-Newton has resulted in revolutionary studies of the Galactic neighborhood in the soft (<10 keV) X-ray band, there are many open questions. We discuss these issues and how they would be addressed by very wide-area (> 100 sq. deg.) X-ray surveys.

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