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We present Log N -- Log S distribution for close-by young isolated neutron stars. On the basis of this distribution it is shown that the seven ROSAT isolated neutron stars (if they are young cooling objects) are genetically related to the…

Astrophysics · Physics 2007-05-23 S. B. Popov , M. E. Prokhorov , M. Colpi , A. Treves , R. Turolla

This review is devoted to studies of the Gould belt and the Local system. Since the Gould belt is the giant stellar-gas complex closest to the sun, its stellar component is characterized, along with the stellar associations and diffuse…

Astrophysics of Galaxies · Physics 2015-07-24 V. V. Bobylev

We suggest that the seven radio-quiet isolated neutron stars observed with ROSAT are young cooling objects associated to recent near-by supernova explosions which formed runaway stars and the Local Bubble, affecting the topology of the…

Astrophysics · Physics 2007-05-23 S. B. Popov , M. E. Prokhorov , M. Colpi , A. Treves , R. Turolla

We present new population synthesis calculations of close young neutron stars. In comparison with our previous investigation we use a different neutron star mass spectrum and different initial spatial and velocity distributions. The results…

Astrophysics · Physics 2009-11-07 S. B. Popov , R. Turolla , M. E. Prokhorov , M. Colpi , A. Treves

Important results achieved over the last years on supernova remnants, planetary nebulae and superbubbles are briefly reviewed in the context of X-ray observations. I intend to review the important open scientific questions in these fields,…

Astrophysics · Physics 2009-06-23 Anne Decourchelle

The recent identification of several groups of young stars within 100 parsecs of the Sun has generated widespread interest. Given their proximity and possible age differences, these systems are ideally suited for detailed studies of disk…

Astrophysics · Physics 2007-05-23 Ray Jayawardhana

Gould's Belt is a flat local system composed of young OB stars, molecular clouds and neutral hydrogen within 500 pc from the Sun. It is inclined about 20 degrees to the galactic plane and its velocity field significantly deviates from…

Astrophysics of Galaxies · Physics 2018-04-25 Jan Palouš , Soňa Ehlerová

We describe properties and gravitational interactions of meteor-mass and greater compact ultra dense objects with nuclear density or greater (CUDO s). We discuss possible enclosure of CUDO s in comets, stability of these objects on impact…

Earth and Planetary Astrophysics · Physics 2013-03-20 J. Rafelski , Ch. Dietl , L. Labun

For the past 150 years, the prevailing view of the local Interstellar Medium (ISM) was based on a peculiarity known as the Gould's Belt, an expanding ring of young stars, gas, and dust, tilted about 20$^\circ$ to the Galactic plane. Still,…

We report first results on the large-scale distribution of the ROSAT All-Sky Survey (RASS) X-ray sources in a 5000 deg^2 field centered on Orion. Our final aim is to study the properties of different widespread populations in the Orion…

Solar and Stellar Astrophysics · Physics 2011-10-18 K. Biazzo , J. M. Alcalá , M. F. Sterzik , E. Covino , A. Frasca , P. Guillout

If the Sun was born in a relatively compact open cluster, it is quite likely that a massive (10MSun) star was nearby when it exploded in a supernova. The repercussions of a supernova can be rather profound, and the current Solar System may…

Solar and Stellar Astrophysics · Physics 2018-08-22 Simon Portegies Zwart , Inti Pelupessy , Arjen van Elteren , Thomas Wijnen , Maria Lugaro

The history of the local medium, within a few hundred parsecs, is dominated by the evolution of the Gould Belt. The event that triggered this star-forming region and molded the gas distribution is still unknown. Its orientation and extent…

Astrophysics · Physics 2007-05-23 Isabelle A. Grenier

Recent developments in the spectropolarimetric study of compact objects, specifically black holes (stellar and massive) and neutron stars are reviewed. The lectures are organized around five topics: disks, jets, outflows, neutron stars and…

Astrophysics · Physics 2007-05-23 Roger Blandford , Eric Agol , Avery Broderick , Jeremy Heyl , Leon Koopmans , Hee-Won Lee

The latest results in the research of forming planetary systems have led several authors to compile a sample of candidates for searching for planets in the vicinity of the sun. Young stellar associations are indeed excellent laboratories…

Astrophysics · Physics 2009-11-11 J. Lopez-Santiago , D. Montes , I. Crespo-Chacon , M. J. Fernandez-Figueroa

Supernova blasts envelop many surrounding stellar systems, transferring kinetic energy to small bodies in the systems. Geologic evidence from $^{60}\rm Fe$ points to recent nearby supernova activity within the past several Myr. Here, we…

Solar and Stellar Astrophysics · Physics 2024-10-17 Leeanne Smith , Jesse A. Miller , Brian D. Fields

Recent high energy gamma-ray observations of both single supernova remnants and superbubbles, together with observations of supernovae, star formation regions, and local cosmic ray composition, now provide an integrated framework tying…

High Energy Astrophysical Phenomena · Physics 2018-10-31 Richard E. Lingenfelter

Extreme magnifications of distant objects by factors of several thousand have recently become a reality. Small very luminous compact objects, such as supernovae (SNe), giant stars at z=1-2, Pop III stars at z>7 and even gravitational waves…

Astrophysics of Galaxies · Physics 2019-05-22 Jose M. Diego

Monte Carlo simulations of Galactic Supernovae are carried out to study the rate of nearby events, which may have a direct effect on Earth's ecology though ionizing radiation and cosmic ray bombardment. A nearby supernova may have left a…

Astrophysics · Physics 2007-05-23 D. H. Hartmann , K. Kretschmer , R. Diehl

The last decade has been dense with new developments in the search for the sources of Galactic cosmic rays. Some of these developments have confirmed the tight connection between cosmic rays and supernovae in our Galaxy, through the…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Pasquale Blasi

The nearby, 30 to 40 Myr old, starburst region of the Gould Belt has formed numerous massive stars. Within its 300 pc radius, it produces core-collapse supernovae at an enhanced rate which is shown to be 75 to 95 Myr{-1} kpc{-2}, i.e. 3 to…

Astrophysics · Physics 2016-08-30 I. A. Grenier
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