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The Global ETD Search service is a free service for researchers
to find electronic theses and dissertations. This service is
provided by the
Networked Digital Library of Theses and Dissertations.
Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
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Showing 11 to 20 of 32 (0.071 seconds)Spelling suggestions: "subject:"accretion (astrophysics)"" "subject:"accretion (petrophysics)""
| 11 |
X-ray reverberation around accreting black holesKara, Erin January 2016 (has links)
No description available.
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| 12 |
Unification of QSOs via black hole and accretion propertiesYuan, Michael Juntao 28 August 2008 (has links)
Not available / text
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| 13 |
Unification of QSOs via black hole and accretion propertiesYuan, Michael Juntao 08 August 2011 (has links)
Not available / text
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| 14 |
X-ray emission and reflection from accreting black holesWalton, Dominic James January 2012 (has links)
No description available.
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| 15 |
Modelling the X-ray spectra of accreting black holesChiang, Chia-Ying January 2013 (has links)
No description available.
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| 16 |
The dynamics of spiral density waves in turbulent accretion discsHeinemann, Tobias January 2010 (has links)
No description available.
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| 17 |
Analysis of the radial profile emissivity of accretion disks in cataclysmic variablesHillwig, Todd C. January 1995 (has links)
There is no abstract available for this thesis. / Department of Physics and Astronomy
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| 18 |
Time-resolved spectroscopy of the AM Herculis-type binary systems QQ VUL and EF ERIBlakelock, Carolyn J. January 1998 (has links)
Cataclysmic variable stars (CVs) are interacting binary systems. One of the stars (referred to as the primary) is a white dwarf, the other (referred to as the secondary) is usually a late main sequence star such as a red dwarf. Due to the closeness of the two stars, the white dwarf accretes gasses from the secondary. If the white dwarf does not possess a strong magnetic field, these gasses go into orbit, forming an accretion disk around the primary. If the white dwarf does possess a strong magnetic field, the gasses cannot form an accretion disk because they are entrained by the magnetic field lines. Cataclysmic variable stars in which the magnetic field is strong enough to prevent the formation of the accretion disk are called AM Herculis-type systems, after their prototype. In this study, the time-resolved spectroscopy of two AM Herculis-type binary systems, QQ Vul and EF Eri, are analyzed. In addition, Doppler Tomography, an analysis technique previously applied primarily to cataclysmic variable stars with accretion disks, is applied to these systems. / Department of Physics and Astronomy
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| 19 |
A multiwavelength analysis of the dwarf nova AR AndromedaWeindorfer, Kimberly J. January 1999 (has links)
There is no abstract available for this thesis. / Department of Physics and Astronomy
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| 20 |
On the global stability of magnetized accretion disks.Curry, Charles Leo. Pudritz, R.E. Unknown Date (has links)
Thesis (Ph.D.)--McMaster University (Canada), 1995. / Source: Dissertation Abstracts International, Volume: 57-03, Section: B, page: 1856. Adviser: R. E. Pudritz.
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