Physical processes in the strong magnetic fields of accreting neutron stars

P. Mészáros

doi:10.1016/0273-1177(84)90104-2

Physical processes in the strong magnetic fields of accreting neutron stars

P. Mészáros

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.

Original language	English (US)
Pages (from-to)	279-285
Number of pages	7
Journal	Advances in Space Research
Volume	3
Issue number	10-12
DOIs	https://doi.org/10.1016/0273-1177(84)90104-2
State	Published - 1984

All Science Journal Classification (ASJC) codes

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
General Earth and Planetary Sciences

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10.1016/0273-1177(84)90104-2

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title = "Physical processes in the strong magnetic fields of accreting neutron stars",

abstract = "The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.",

author = "P. M{\'e}sz{\'a}ros",

note = "Funding Information: *Smithsonian Visiting Scientist\textasciitilde{} on leave from Max-Planck-Institut fur Physik and Astrophysik I\textasciitilde{}E; partly supported by NASA NA\textasciitilde{}q-246",

year = "1984",

doi = "10.1016/0273-1177(84)90104-2",

language = "English (US)",

volume = "3",

pages = "279--285",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Ltd",

number = "10-12",

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T1 - Physical processes in the strong magnetic fields of accreting neutron stars

AU - Mészáros, P.

N1 - Funding Information: *Smithsonian Visiting Scientist~ on leave from Max-Planck-Institut fur Physik and Astrophysik I~E; partly supported by NASA NA~q-246

PY - 1984

Y1 - 1984

N2 - The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.

AB - The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.

UR - https://www.scopus.com/pages/publications/48749136321

UR - https://www.scopus.com/pages/publications/48749136321#tab=citedBy

U2 - 10.1016/0273-1177(84)90104-2

DO - 10.1016/0273-1177(84)90104-2

M3 - Article

AN - SCOPUS:48749136321

SN - 0273-1177

VL - 3

SP - 279

EP - 285

JO - Advances in Space Research

JF - Advances in Space Research

IS - 10-12

ER -

Physical processes in the strong magnetic fields of accreting neutron stars

Abstract

All Science Journal Classification (ASJC) codes

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