A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray Luminous Classical Nova to Date

It has recently been discovered that some, if not all, classical novae emit GeV gamma rays during outburst, but the mechanisms involved in the production of the gamma rays are still not well understood. We present here a comprehensive multi-wavelength dataset---from radio to X-rays---for the most ga...

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Veröffentlicht in:	arXiv.org 2017-11
Hauptverfasser:	Finzell, Thomas, Chomiuk, Laura, Metzger, Brian D, Walter, Frederick M, Linford, Justin D, Mukai, Koji, Nelson, Thomas, Weston, Jennifer H S, Zheng, Yong, Sokoloski, Jennifer L, Mioduszewski, Amy, Rupen, Michael P, Dong, Subo, Sumner Starrfield, Cheung, C C, Bohlsen, Terry, Woodward, Charles E, Taylor, Gregory B, Buil, Christian, Prieto, Jose, Wagner, R Mark, Bensby, Thomas, Bond, I A, Sumi, T, Bennett, D P, Abe, F, Koshimoto, N, Suzuki, D, P, Tristram, J, Christie, Grant W, Natusch, Tim, McCormick, Jennie, Yee, Jennifer, Gould, Andy
Format:	Artikel
Sprache:	eng
Schlagworte:	Ejecta Gamma rays Light curve Novae Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics
Online-Zugang:	Volltext
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