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Understanding neutron stars using thermonuclear x-ray bursts
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Bhattacharyya, S. |
| Copyright Year | 2007 |
| Description | Studies of thermonuclear X-ray bursts can be very useful to constrain the spin rate, mass and radius of a neutron star = EOS model of high density cold matter in the neutron star cores. Extensive observation and analysis of the data from the rising portions of the bursts = modeling of burst oscillations and thermonuclear flame spreading. Theoretical study of thermonuclear flame spreading on the rapidly spinning neutron stars should be done considering all the main physical effects (including magnetic field, nuclear energy generation, Coriolis effect, strong gravity, etc.). |
| File Size | 682122 |
| Page Count | 26 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20080032436 |
| Archival Resource Key | ark:/13960/t75t8mb0h |
| Language | English |
| Publisher Date | 2007-09-18 |
| Access Restriction | Open |
| Subject Keyword | Extraterrestrial Matter Flames Neutron Stars Gravitation X Rays Spreading Oscillations Magnetic Fields Coriolis Effect Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
