Zobrazeno 1 - 10
of 113
pro vyhledávání: '"Julian M. Pittard"'
Autor:
Theodore R. Gull, Felipe Navarete, Michael F. Corcoran, Augusto Damineli, David Espinoza, Kenji Hamaguchi, Henrik Hartman, D. John Hillier, Thomas Madura, Anthony F. J. Moffat, Patrick Morris, Krister Nielsen, Julian M. Pittard, Andrew M. T. Pollock, Noel D. Richardson, Christopher M. P. Russell, Ian R. Stevens, Gerd Weigelt
Since 2002, the far-ultraviolet (FUV) flux (1150–1680 Å) of Eta Carinae, monitored by the Hubble Space Telescope/Space Telescope Imaging Spectrograph, has increased by an order of magnitude. This increase is attributed to partial dissipation of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18d7c6ff12756c3779516f757298ebd9
https://resolver.caltech.edu/CaltechAUTHORS:20220107-81089900
https://resolver.caltech.edu/CaltechAUTHORS:20220107-81089900
We present a model for the creation of non-thermal particles via diffusive shock acceleration in a colliding-wind binary. Our model accounts for the oblique nature of the global shocks bounding the wind-wind collision region and the finite velocity o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d392f59180660ea4043ccbe05a3c49ef
https://eprints.whiterose.ac.uk/175334/1/2104.07399v1.pdf
https://eprints.whiterose.ac.uk/175334/1/2104.07399v1.pdf
Using the adaptive mesh refinement code mg, we perform hydrodynamic simulations of the interaction of a shock with a molecular cloud evolving due to thermal instability (TI) and gravity. To explore the relative importance of these processes, three ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88dd5e1987d3f9011cdc2c282fd89139
https://eprints.whiterose.ac.uk/169465/1/2012.04546v1.pdf
https://eprints.whiterose.ac.uk/169465/1/2012.04546v1.pdf
Stellar winds are one of several ways that massive stars can affect the star formation process on local and galactic scales. In this paper we investigate the numerical resolution needed to inflate an energy-driven stellar wind bubble in an external m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2dd64d799613c3a10161090d79368d4c
The MHD version of the adaptive mesh refinement (AMR) code, MG, has been employed to study the interaction of thermal instability, magnetic fields and gravity through 3D simulations of the formation of collapsing cold clumps on the scale of a few par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a47c535ba8914a73bebe1c611cbbdbd
https://eprints.whiterose.ac.uk/167579/1/ms2020_magcollapse_R3.pdf
https://eprints.whiterose.ac.uk/167579/1/ms2020_magcollapse_R3.pdf
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We present a model for the non-thermal emission from a colliding-wind binary. Relativistic protons and electrons are assumed to be accelerated through diffusive shock acceleration (DSA) at the global shocks bounding the wind-wind collision region. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab96318593a2cfadabcf1dad1afe6b95
https://academic.oup.com/mnras/article/495/2/2205/5824173
https://academic.oup.com/mnras/article/495/2/2205/5824173
Autor:
Nicholas J. Wright, Sean M. Dougherty, J. S. Clark, Jeremy Yates, R. K. Prinja, H. A. Smith, Danielle Fenech, Jorick S. Vink, Anita M. S. Richards, Jeremy J. Drake, Julian M. Pittard, Ian R. Stevens, Ronny Blomme, S. P. S. Eyres, J. C. Morford
Publikováno v:
Morford, J C, Fenech, D M, Prinja, R K, Blomme, R, Yates, J A, Drake, J J, Eyres, S P S, Richards, A M S, Stevens, I R, Wright, N J, Clark, J S, Dougherty, S, Pittard, J M, Smith, H & Vink, J S 2020, ' COBRaS : The e-MERLIN 21 cm Legacy survey of Cygnus OB2 ', A&A, vol. 637, A64 . https://doi.org/10.1051/0004-6361/201731379
The role of massive stars is central to an understanding of galactic ecology. It is important to establish the details of how massive stars provide radiative, chemical, and mechanical feedback in galaxies. Central to these issues is an understanding
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad4221916ca7808a109eeaca722471e7
https://doi.org/10.1051/0004-6361/201731379
https://doi.org/10.1051/0004-6361/201731379
Field's linear analysis of thermal instability is repeated using methods related to Whitham's theory of wave hierarchies, which brings out the physically relevant parameters in a much clearer way than in the original analysis. It is also used for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4410422f18d5bcc3cef963080d1b8f31
Cyg OB2 #8a is a massive O-type binary displaying strong non-thermal radio emission. Owing to the compactness of this binary, emission of non-thermal X-ray photons via inverse Compton scattering is expected. We first revised the orbital solution for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::913aaf0a5655659c4d4e21310eef477c
Autor:
Julian M. Pittard, B. Dawson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:5640-5645
We investigate the structure and X-ray emission from the colliding stellar winds in massive star binaries. We find that the opening angle of the contact discontinuity (CD) is overestimated by several formulae in the literature at very small values of