neutron starsnuclear forcesnuclear matterstellar massstellar rotation/ hot neutron starTolmann-Oppenheimer-Volkoff equationneutron matterdensity dependent Sussex interactionThe properties of neutron star at temperatures 5 MeV, 10 MeV and15 MeV are calculated by solving Tolmannu2013Oppenheimeru2013Volkoff (...
Stars much more massive than the Sun have a slightly different fate. While the Sun's mass is only sufficient to fuse lighter elements, a star that is around 8 times the mass of our Sun will have the energy to fuse many heavier elements. Towards the end of their lives, these massive s...
Emission properties of compact astrophysical objects such as Neutron stars (NSs) are associated with crucial astronomical observables. In the current work,
P. A. CrowtherDepartment of Physics and AstronomyUniversity College LondonMonthly Notices of the Royal Astronomical SocietyDe Marco, O., Barlow, M.J. and Storey, P.J.: 1997, The WC10 central stars CPD-56deg8032 and He 2-113-I. Distances and nebular parameters MNRAS , 292 , 86-104....
With increasing surface coverage, two first-order phase transitions are also described in the films of stars with stiff chains. One of them is an order-disorder transition in the dense layers parallel to the surface, packed by floating branches. The other transition, from a monolayer with ...
infrared : starsISM : individual (OMC-2, OMC-3stars : pre-main-sequenceX-rays : starsWe report X-ray results of the Chandra observation of OMC-2 and OMC-3. A deep exposure of ～ 100 ks detects ～ 400 X-ray sources in the field of view of the ACIS array, providing one of the ...
S. Komossa, Ludwig Biermann award lecture: X-ray evidence for supermassive black holes at the centers of nearby, non-active galaxies. Rev. Mod. Astron. 15, 27 (2002) ADS Google Scholar S. Komossa, The extremes of (X-ray) variability among galaxies: flares from stars tidally disrupted...
, Planets, Stars and Nebulae Studied with Photo polarimetry, University of Arizona, Tucson, in press. Google Scholar Briggs, F. H.: 1973, Astrophys. J. 182, 999. Google Scholar Brinkmann, R. T.: 1973, Icarus 19, 15. Google Scholar Brinkmann, R. T. and Millis, R. L.: 1973,...
SEMIFLEXIBLE STARS This section addresses semiflexible (regular) star polymers. Goodson and Novak7 synthesized three-arm star poly(n-hexyl isocyanate), which is a typical semiflexible polymer, by living titanium-catalyzed coordination polymerization. The three-arm star poly(n-hexyl Department of ...
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