arXiv · 2105.13911
A Search for TeV Gamma-ray Emission from Pulsar Tails by VERITAS
Abstract
We report on the search for very-high-energy gamma-ray emission from the regions around three nearby supersonic pulsars (PSR B0355+54, PSR J0357+3205 and PSR J1740+1000) that exhibit long X-ray tails. To date there is no clear detection of TeV emission from any pulsar tail that is prominent in X-ray or radio. We provide upper limits on the TeV flux, and luminosity, and also compare these limits with other pulsar wind nebulae detected in X-rays and the tail emission model predictions. We find that at least one of the three tails is likely to be detected in observations that are a factor of 2-3 more sensitive. The analysis presented here also has implications for deriving the properties of pulsar tails, for those pulsars whose tails could be detected in TeV.
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Wystan Benbow, A. Brill, James Buckley, M Capasso, A Chromey, M. Errando, Abraham Falcone, K. A. Farrell, Qi Feng, J Finley, G. M. Foote, Lucy Fortson, Amy Furniss, Alasdair Gent, C Giuri, David Hanna, Tarek Hassan, Olivier Hervet, Jamie Holder, G Hughes, T. B. Humensky, Weidong Jin, Philip Kaaret, Oleg Kargaltsev, Mary P. Kertzman, David Kieda, Noel Klingler, Sajan Kumar, M Lang, M Lundy, Gernot Maier, C. E. McGrath, Patrick Moriarty, Reshmi Mukherjee, D Nieto, M Nievas-Rosillo, S O'Brien, Rene A. Ong, A. N. Otte, S. Patel, Konstantin Pfrang, Martin Pohl, Raul Prado, John Quinn, Kenneth J. Ragan, P., T. Reynolds, D Ribeiro, G. T. Richards, Emmet Thomas Roache, James Ryan, Marcos Santander, Glenn H Sembroski, R Shang, Igor Volkov, S. P Wakely, Amanda Weinstein, P. Wilcox, D. A. Williams. 2021-05-28. A Search for TeV Gamma-ray Emission from Pulsar Tails by VERITAS. https://doi.org/10.3847/1538-4357%2Fac05b9
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