Radiation pressure-driven magnetic disk winds in broad absorption line quasi-stellar objects
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Radiation pressure-driven magnetic disk winds in broad absorption line quasi-stellar objects

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Published by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va .
Written in English

Subjects:

  • Accretion disks,
  • Quasars,
  • X ray absorption,
  • Magnetic fields,
  • Line spectra,
  • Confinement,
  • Radiation pressure

Book details:

Edition Notes

Other titlesRadiation pressure driven magnetic disk winds in broad absorption line quasi-stellar objects.
StatementMartin De Kool and Mitchell C. Begelman.
Series[NASA contractor report] -- NASA-CR-204982., NASA contractor report -- NASA CR-204982.
ContributionsBegelman, Mitchell C., United States. National Aeronautics and Space Administration.
The Physical Object
FormatMicroform
Pagination1 v.
ID Numbers
Open LibraryOL17834344M
OCLC/WorldCa39348159

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Buy Radiation pressure-driven magnetic disk winds in broad absorption line quasi-stellar objects (SuDoc NAS ) by Martin De Kool (ISBN:) from Amazon's Book Store. Everyday low prices and free delivery on eligible : De Kool, Martin. We use cookies to offer you a better experience, personalize content, tailor advertising, provide social media features, and better understand the use of our services. de Kool M, Begelman MC () Radiation Pressure-driven Magnetic Disk Winds in Broad Absorption Line Quasi-stellar Objects. ApJ doi: / ADS CrossRef Google Scholar Decarli R, Labita M, Treves A, Falomo R () On the geometry of broad emission region in by: Radiation-driven warping: The origin of warps and precession in accretion disks. Self-consistent thermal accretion disk corona models for compact objects RADIATION PRESSURE-DRIVEN MAGNETIC DISK WINDS IN BROAD ABSORPTION-LINE QUASI-STELLAR OBJECTS.

Line-driven disk winds in active galactic nuclei Article in Advances in Space Research 28(2) July with 7 Reads How we measure 'reads'. de Kool M, Begelman MC () Radiation Pressure-driven Magnetic Disk Winds in Broad Absorption Line Quasi-stellar Objects. ApJ doi: . Due to the need to contain the spread of coronavirus (COVID) the Library building and reading rooms are closed to visitors until further notice. Hydrodynamic ejection of bipolar flows from objects undergoing disk accretion: T Tauri stars, massive pre-main-sequence objects, and cataclysmic variables.

  A revised and updated catalog of quasi-stellar objects. NASA Technical Reports Server (NTRS) Hewitt, A.; Burbidge, G. The paper contains a . This page intentionally left blank THE EMI SSI ON- LI NE UNI VERSE Emission lines provide a powerful tool for studying the physical properties and chemical compositions of astroph. The broad-band X-ray spectrum is fitted with a dominant emission temperature of just kT= keV along with significant wind absorption. The broad-band wind absorption and the line profiles provide two independent measurements of the wind mass-loss rate: + × M ☉ yr-1 and + × M ☉ yr-1, respectively. This is. Rotational periods increase with stellar age, as expected for a magnetic braking scenario. Without exception, all stars with H α emission originating in a CM are (1) rapid rotators, (2) strongly magnetic, and (3) young, with the latter property consistent with the observation that magnetic fields and rotation both decrease over time.