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, Katarzynski 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, Marti-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, Puehlhofer 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, Schussler 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, Zywucka N (2019)
Publication Type: Journal article, Original article
Publication year: 2019
Book Volume: 627
Article Number: A100
DOI: 10.1051/0004-6361/201935458
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.
APA:
Abdalla, H., Aharonian, F., Benkhali, F.A., Anguner, E.O., Arakawa, M., Arcaro, C.,... Zywucka, N. (2019). HESS and Suzaku observations of the Vela X pulsar wind nebula. Astronomy & Astrophysics, 627. https://dx.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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