HESS and Suzaku observations of the Vela X pulsar wind nebula

Abdalla H, Aharonian F, Benkhali FA, Anguner EO, Arakawa M, Arcaro C, Armand C, Backes M, Barnard M, Becherini Y, Berge D, Bernloehr K, Blackwell R, Bottcher M, Boisson C, Bolmont J, Bonnefoy S, Bregeon J, Brun F, Brun P, Bryan M, Büchele M, Bulik T, Bylund T, Capasso M, Caroff S, Carosi A, Casanova S, Cerruti M, Chakraborty N, Chand T, Chandra S, Chaves RCG, Chen A, Colafrancesco S, Condon B, Davids ID, Deil C, Devin J, Dewilt P, Dirson L, Djannati-Atai A, Dmytriiev A, Donath A, Doroshenko , Drury LO, Dyks J, Egberts K, Emery G, Ernenwein JP, Eschbach S, Feijen K, Fegan S, Fiasson A, Fontaine G, Funk S, Fuessling M, Gabici S, Gallant YA, Gate F, Giavitto G, Glawion D, Glicenstein JF, Gottschall D, Grondin MH, Hahn J, Haupt M, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hofmann W, Hoischen C, Holch TL, Holler M, Horns D, Huber D, Iwasaki H, Jacholkowska A, Jamrozy M, Jankowsky D, Jankowsky F, Jouvin L, Jung-Richardt I, Kastendieck MA, Katarzyński K, Katsuragawa M, Katz U, Khangulyan D, Khelifi B, King J, Klepser S, Kluzniak W, Komin N, Kosack K, Kostunin D, Kraus M, Lamanna G, Lau J, Lemiere A, Lemoine-Goumard M, Lenain JP, Leser E, Lohse T, Lopez-Coto R, Lypova , Malyshev D, Marandon , Marcowith A, Mariaud C, Martí-Devesa G, Marx R, Maurin G, Maxted N, Meintjes PJ, Mitchell AMW, Moderski R, Mohamed M, Mohrmann L, Moore C, Moulin E, Murach T, Nakashima S, De Naurois M, Ndiyavala H, Niederwanger F, Niemiec J, Oakes L, O'Brien P, Odaka H, Ohm S, Wilhelmi EDO, Ostrowski M, Oya , Panter M, Parsons RD, Perennes C, Petrucci PO, Peyaud B, Piel Q, Pita S, Poireau , Noel AP, Prokhorov DA, Prokoph H, Pühlhofer G, Punch M, Quirrenbach A, Raab S, Rauth R, Reimer A, Reimer O, Renaud M, Rieger F, Rinchiuso L, Romoli C, Rowell G, Rudak B, Ruiz-Velasco E, Sahakian , Saito S, Sanchez DA, Santangelo A, Sasaki M, Schlickeiser R, Schüssler F, Schulz A, Schutte H, Schwanke U, Schwemmer S, Seglar-Arroyo M, Senniappan M, Seyffert AS, Shafi N, Shilon , Shiningayamwe K, Simoni R, Sinha A, Sol H, Specovius A, Spir-Jacob M, Stawarz L, Steenkamp R, Stegmann C, Steppa C, Takahashi T, Tavernet JP, Tavernier T, Taylor AM, Terrier R, Tibaldo L, Tiziani D, Tluczykont M, Trichard C, Tsirou M, Tsuji N, Tuffs R, Uchiyama Y, Van Der Walt DJ, van Eldik C, Van Rensburg C, Van Soelen B, Vasileiadis G, Veh J, Venter C, Vincent P, Vink J, Voisin F, Voelk HJ, Vuillaume T, Wadiasingh Z, Wagner SJ, White R, Wierzcholska A, Yang R, Yoneda H, Zaborov D, Zacharias M, Zanin R, Zdziarski AA, Zech A, Ziegler A, Zorn J, Żywucka N (2019)


Publication Type: Journal article, Original article

Publication year: 2019

Journal

Book Volume: 627

Article Number: A100

DOI: 10.1051/0004-6361/201935458

Abstract

Context. Pulsar wind nebulae (PWNe) represent the most prominent population of Galactic very-high-energy gamma-ray sources and are thought to be an efficient source of leptonic cosmic rays. Vela X is a nearby middle-aged PWN, which shows bright X-ray and TeV gamma-ray emission towards an elongated structure called the cocoon.

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APA:

Abdalla, H., Aharonian, F., Benkhali, F.A., Anguner, E.O., Arakawa, M., Arcaro, C.,... Żywucka, N. (2019). HESS and Suzaku observations of the Vela X pulsar wind nebula. Astronomy & Astrophysics, 627. https://doi.org/10.1051/0004-6361/201935458

MLA:

Abdalla, H., et al. "HESS and Suzaku observations of the Vela X pulsar wind nebula." Astronomy & Astrophysics 627 (2019).

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