Deeper Chandra Follow-up of Cygnus TeV Source Perpetuates Mystery

BUTT, YOUSAF M.; DRAKE, JEREMY; BENAGLIA, PAULA; COMBI, JORGE A.; DAME, THOMAS; MINIATI, FRANCESCO; ROMERO, GUSTAVO E.

ASTROPHYSICAL JOURNAL

The University of Chicago Press

Lugar: Chicago; Año: 2006 vol. 643 p. 238 - 244

0004-637X

A 50 ksec Chandra observation of the unidentified TeV source in Cygnus reported by the HEGRA collaboration reveals no obvious diffuse X-ray counterpart. However, 240 Pointlike X-ray sources are detected within or nearby the extended TeV J2032+4130 source region, of which at least 36 are massive stars and 2 may be radio emitters. That the HEGRA source is a composite, having as counterpart the multiple point-like X-ray sources we observe, cannot be ruled out. Indeed, the distribution of point-like X-ray sources appears non-uniform and concentrated broadly within the extent of the TeV source region. We offer a hypothesis for the origin of the very high energy gamma-ray emission in Cyg OB2 based on the local acceleration of TeV range cosmic rays and the differential distribution of OB vs. less massive stars in this association.