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The Astrophysical Journal
Article . 2014 . Peer-reviewed
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https://dx.doi.org/10.48550/ar...
Article . 2014
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INVESTIGATING THE TeV MORPHOLOGY OF MGRO J1908+06 WITH VERITAS

Authors: E. Aliu; S. Archambault; T. Aune; B. Behera; M. Beilicke; W. Benbow; K. Berger; +81 Authors

INVESTIGATING THE TeV MORPHOLOGY OF MGRO J1908+06 WITH VERITAS

Abstract

We report on deep observations of the extended TeV gamma-ray source MGRO J1908+06 made with the VERITAS very high energy (VHE) gamma-ray observatory. Previously, the TeV emission has been attributed to the pulsar wind nebula (PWN) of the Fermi-LAT pulsar PSR J1907+0602. We detect MGRO J1908+06 at a significance level of 14 standard deviations (14 sigma) and measure a photon index of 2.20 +/- 0.10_stat +/- 0.20_sys. The TeV emission is extended, covering the region near PSR J1907+0602 and also extending towards SNR G40.5--0.5. When fitted with a 2-dimensional Gaussian, the intrinsic extension has a standard deviation of sigma_src = 0.44 +/- 0.02 degrees. In contrast to other TeV PWNe of similar age in which the TeV spectrum softens with distance from the pulsar, the TeV spectrum measured near the pulsar location is consistent with that measured at a position near the rim of G40.5--0.5, 0.33 degrees away.

To appear in ApJ, 8 pages

Countries
Ireland, Ireland, Germany
Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), gamma-ray burst: individual (mgro j1908+06, ver j1907+062), Institut für Physik und Astronomie, g40.5-0.5, FOS: Physical sciences, gamma rays: general, array, gamma-ray burst: individual (mgro j1908+06, gamma-ray emission, galactic plane, 520, remnant, milagro, pulsars: individual (psr j1907+0602), psr j1907+0602, ism: supernova remnants, ver j1907+062), pulsar wind nebula, Astrophysics - High Energy Astrophysical Phenomena, ddc: ddc:520

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
36
Top 10%
Top 10%
Top 10%
Green
gold