The Galactic distribution velocities luminosities and evolution of pulsars

Download
038605.pdf
1995
Gök, Fatma
Show full item record
85
views
0
downloads
Pulsars, Stars
https://hdl.handle.net/11511/1077
Graduate School of Natural and Applied Sciences, Thesis

Suggestions

The Pre-main sequence evolutionary models of low mass stars in the mass range 0.30 M. - 0.60 M.
Küçük, İbrahim; Eryurt Ezer, Dilhan; Department of Physics (1993)
Evolution of a rotating component star.
Çelikel, F Rikkat; Eryurt Ezer, Dilhan; Department of Physics (1987)
The timing noise of PSR 0823+26, 1706-16, 1749-28, 2021+51 and the anomalous braking indices
Baykal, Altan; Boynton, PE; Deeter, JE (1999-06-11)
We have investigated the stability of the pulse frequency second derivatives (ii) of PSR 0823+26, 1706-16, 1749-28 and 2021+51 that show significant quadratic trends in their pulse-frequency histories in order to determine whether the observed second derivatives are secular or if they arise as part: of noise processes. We have used time-of-arrival (TOA) data extending to more than three decades, which are the longest time-spans ever taken into account in pulse-timing analyses. We investigated the stability ...
Determining the asymmetry in supernova explosions by studying the radial velocities of OB runaway stars
Dinçel, Baha; Yerli, Sinan Kaan; Ankay, Aşkın; Department of Physics (2012)
Understanding the asymmetry in core collapse supernova explosions is pointed out by various astrophysicists as it is the key factor in determining the observational properties of the pulsars. The initial kick given by the ex- plosion to the pulsar affects its spin period and space velocity. Up to now, although the observations do not show a direct relation between the observational features of the pulsar and its space velocity, they show a clear relation between the spin period and the magnetic field streng...
The Spectral and temporal properties of MAXI J1409-619
Dönmez, Çağatay Kerem; Baykal, Altan; Department of Physics (2019)
In this thesis, spectral and timing analysis of the transient high-mass X-ray binary (HMXB) pulsar MAXI J1409-619 are presented. MAXI J1409-619 was discovered in October 2010, and went into an outburst in early December 2010 until February 2011. Observations of Swift and RXTE throughout this period are used in the thesis. The analysis results are in line with the assertion that MAXI J1409-619 is an accretion-powered pulsar. Time-resolved energy spectra of RXTE and Swift data confirm the previously reported ...
Citation Formats
F. Gök, “The Galactic distribution velocities luminosities and evolution of pulsars,” Ph.D. - Doctoral Program, Middle East Technical University, 1995.
METU IIS - Integrated Information Service open@metu.edu.tr