Results 1 to 10 of about 8,188 (190)

The Pulsar Wind Nebula of the Geminga Pulsar [PDF]

The Astrophysical Journal, 2006
Revised version: data analysis described in more detail, Figure 2 replaced; 6 pages, 2 color figures; accepted for publication in ApJ (v.643, 2006 June 1)
George G. Pavlov, D. Sanwal, V. E. Zavlin   +2 more
openalex   +4 more sources

The Pulsar Wind Nebula in G11.2−0.3 [PDF]

The Astrophysical Journal, 2003
4 pages, 2 figures, To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B.
M. S. Roberts, Cindy R. Tam, V. M. Kaspi, Maxim Lyutikov, Gautam Vasisht, M. J. Pivovaroff, E. V. Gotthelf, N. Kawai   +7 more
openalex   +6 more sources

Resolving the Crab pulsar wind nebula at teraelectronvolt energies [PDF]

Nature Astronomy, 2019
23 pages, 5 ...
H. Abdalla, F. Aharonian, F. Ait Benkhali, E. O. Angüner, Masanori Arakawa, Cornelia Arcaro, Céline Armand, Michael Backes, M. Barnard, Y. Becherini, J. Becker Tjus, D. Berge, K. Bernlöhr, R. Blackwell, M. Böttcher, C. Boisson, J. Bolmont, S. Bonnefoy, P. Bordas, J. Bregeon, F. Brun, P. Brun, M. Bryan, M. Büchele, T. Bulik, T. Bylund, M. Capasso, Sami Caroff, A. Carosi, S. Casanova, M. Cerruti, Nachiketa Chakraborty, T. Chand, S. Chandra, R. C. G. Chaves, A. Chen, S. Colafrancesco, B. Condon, I. D. Davids, C. Deil, J. Devin, P. deWilt, L. Dirson, A. Djannati-Ataı̈, A. Dmytriiev, Axel Donath, Victor Doroshenko, L. O’C. Drury, J. Dyks, K. Egberts, G. Emery, J.-P. Ernenwein, S. Eschbach, S. Fegan, A. Fiaßon, G. Fontaine, S. Funk, M. Füßling, S. Gabici, Y. A. Gallant, F. Gaté, G. Giavitto, D. Glawion, J. F. Glicenstein, D. Gottschall, M.-H. Grondin, Joachim Hahn, M. Haupt, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, W. Hofmann, C. Hoischen, T. L. Holch, M. Holler, D. Horns, David Miles Huber, H. Iwasaki, A. Jachołkowska, M. Jamrozy, D. Jankowsky, F. Jankowsky, L. Jouvin, I. Jung-Richardt, M. A. Kastendieck, K. Katarzyński, M. Katsuragawa, U. Katz, D. Khangulyan, B. Khélifi, J. King, S. Klepser, W. Kluźniak, Nu. Komin, K. Kosack, M. Kraus, G. Lamanna, J. Lau, J. Lefaucheur   +99 more
openalex   +13 more sources

Ultra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula [PDF]

Innovation (Camb)

openalex   +2 more sources

Why (Still) Studying Turbulence in Fluids and Plasmas?

Perspectives of Earth and Space Scientists, Volume 4, Issue 1, December 2023., 2023
Abstract Turbulence, a captivating and intricate phenomenon, continues to attract researchers across diverse scientific disciplines. Despite considerable efforts, turbulence remains a fascinating challenge and stands as one of the unsolved enigmas in classical physics.
Tommaso Alberti, Roberto Benzi, Vincenzo Carbone   +2 more
wiley   +1 more source

Long‐Term Density Trend in the Mesosphere and Lower Thermosphere From Occultations of the Crab Nebula With X‐Ray Astronomy Satellites

Journal of Geophysical Research: Space Physics, Volume 128, Issue 2, February 2023., 2023
Abstract We present long‐term density trends of the Earth's upper atmosphere at altitudes between 71 and 116 km, based on atmospheric occultations of the Crab Nebula observed with X‐ray astronomy satellites, ASCA, RXTE, Suzaku, NuSTAR, and Hitomi. The combination of the five satellites provides a time period of 28 years from 1994 to 2022.
Satoru Katsuda, Teruaki Enoto, Andrea N. Lommen, Koji Mori, Yuko Motizuki, Motoki Nakajima, Nathaniel C. Ruhl, Kosuke Sato, Gunter Stober, Makoto S. Tashiro, Yukikatsu Terada, Kent S. Wood   +11 more
wiley   +1 more source

A search for runaway stars in 12 Galactic supernova remnants

Astronomische Nachrichten, Volume 342, Issue 3, Page 553-577, March 2021., 2021
Runaway stars can result from core‐collapse supernovae in multiple stellar systems. If the supernova disrupts the system, the companion is ejected with its former orbital velocity. A clear identification of a runaway star can yield the time and place of the explosion, as well as orbital parameters of the pre‐supernova binary system.
Oliver Lux, Ralph Neuhäuser, Markus Mugrauer, Richard Bischoff   +3 more
wiley   +1 more source

Theory of Pulsar Wind Nebulae [PDF]

AIP Conference Proceedings, 2008
Our understanding of Pulsar Wind Nebulae (PWNe), has greatly improved in the last years thanks to unprecedented high resolution images taken from the HUBBLE, CHANDRA and XMM satellites. The discovery of complex but similar inner features, with the presence of unexpected axisymmetric rings and jets, has prompted a new investigation into the dynamics of ...
Cumming, A., Bassa, C., Bucciantini, N., Bucciantini, N., Kaspi, V., Wang, Z.   +5 more
openaire   +3 more sources

Pulsar Wind Nebulae

, 2022
Invited chapter for the "Handbook of X-ray and Gamma-ray Astrophysics" (Springer) Editors C. Bambi & A. Santangelo. Accepted.
Mitchell, A. M. W., Gelfand, J.
openaire   +2 more sources

The Mouse Pulsar Wind Nebula [PDF]

The Astrophysical Journal, 2018
Abstract The young energetic pulsar J1747–2958 (τ = 26 kyr, erg s−1) powers the Mouse pulsar wind nebula (PWN), famous for its spectacular tail spanning 45″ in X-rays and 12′ in radio (d ∼ 5 kpc).
Noel Klingler, Oleg Kargaltsev, George G. Pavlov, C.-Y. Ng, Paz Beniamini, Igor Volkov   +5 more
openaire   +4 more sources