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'Pulsars' web sites

www.symmetrymagazine.org
Fermi telescope finds more new pulsars. symmetry magazine
2016-01-07
pulsars . symmetry magazine Skip to main content Topics Higgs boson Neutrinos Dark matter Dark energy New physics Applications Full archive Follow Search A joint Fermilab SLAC publication Fermi Telescope finds more new pulsars November 02, 2009 Clouds of charged particles move along the pulsar 39;s magnetic field lines blue and create a lighthouse.like beam of gamma rays purple in this illustration. Credit NASA Today at the 2009
astro.fnal.gov
Fermilab center for particle astrophysics
2013-03-21 ⚑music
pulsars too faint to be detected individually, but perhaps collectively bright enough to make up this gamma.ray signal. This interpretation is a bit strained, however, by the degree of isotropy that is exhibited by the gamma.ray background. If enough bright pulsars were present far away from the Galactic Plane to make up the signal from the bubbles, then one would expect the gamma.ray background to be less isotropic than is
www.arxiv.org
Http://www.arxiv.org/abs/1302.6589
2016-01-08
pulsars as a possible astrophysical explanation for the signal, as observed millisecond pulsars possess a spectral cutoff at approximately the required energy. Any such scenario would require a large population of unresolved millisecond pulsars extending at least 2.3 kpc from the GC. Comments 26 pages, 20 figures Subjects High Energy Astrophysical Phenomena astro.ph.HE ; Cosmology and Nongalactic Astrophysics astro.ph.CO ; High
boinc.berkeley.edu
Http://boinc.berkeley.edu
2016-04-01
pulsars , and do many other types of scientific research. It safe, secure, and easy Choose projects Download BOINC software Enter an email address and password. Or, if you run several projects, try an account manager such as GridRepublic or BAM. For Android devices, download the BOINC app from the Google Play Store or for Kindle the Amazon App Store. Compute with BOINC Documentation Software updates Scientists use BOINC to create a
asa.usno.navy.mil
The astronomical almanac online mdash; stars and stellar systems
2015-08-13
pulsars , and gamma ray sources. Some of these tables are made available here. An application to search the list of bright stars by position and magnitude is now available. Bright Stars Double Stars Landolt UBVRI Standard Stars Johnson UBVRI Standard Stars uvby and H Beta; Standard Stars Spectrophotometric Standard Stars Radial Velocity Standard Stars Variable Stars Exoplanets and Host Stars Bright Galaxies Open Clusters Globular
www.aas.org
High energy astrophysics division
2013-03-20
pulsars . Congratulations. Two new members.Daryl Haggard Northwestern University and Henric Krawczynski Washington University in St. Louis. were elected to three.year terms 2013.2016 as members of the HEAD Executive Committee. Congratulations to both. And thanks to retiring members Jack Hughes, Frits Paerels, and Belinda Wilkes. HEAD Officers Chair 2010.2013 Joel Bregman 734 764.3454 Secretary 2012 Randall Smith 617 495.7143
Astronomical subject keywords update october 2009. american astronomical [..]
pulsars general stars pulsars individual..,.. stars rotation stars solar.type stars starspots stars statistics stars subdwarfs stars supergiants stars supernovae general stars supernovae individual..,.. stars variables Cepheids stars variables delta Scuti stars variables general stars variables RR Lyrae stars variables S Doradus stars variables T Tauri, Herbig Ae Be stars white dwarfs stars winds, outflows stars Wolf Rayet
Apj, apjl, apjs aim and scope. american astronomical society
pulsars , neutron stars, black holes, solar and stellar magnetic fields, X.rays, and interstellar matter. The Astrophysical Journal Letters Part 2 The Letters section was created as Part 2 of The Astrophysical Journal in 1967 by S. Chandrasekhar. He cited the need for a separate publishing schedule that allowed astrophysicists to rapidly publish short notices of their spectacular developments in astronomy, S. Chandrasekhar, 1967,
www.space.com
Seti and intelligent design
2014-11-09 ⚑shop
pulsars . stellar objects that flash light and radio waves into space with impressive regularity. pulsars were briefly tagged with the moniker LGM Little Green Men upon their discovery in 1967. Of course, these little men didn t have much to say. Regular pulses don t convey any information.no more than the ticking of a clock. But the real kicker is something else inefficiency. pulsars flash over the entire spectrum. No matter where
About lafayette college
2016-03-12 ⚑r&d
pulsars to measure gravitational waves and ripples in spacetime with his team of student researchers. Meet Professor Nice Our Community BeTheMarquis Join us in celebrating the 190th anniversary of lafayettecollege. To mark the occasion, we re holding a GiveLafayette Challenge, which begins at 8 am today and ends at 8 am March 10. The goal 480 gifts in 48 hours. Every gift, of any amount, makes an impact. lafayettecollege Last
www.jb.man.ac.uk
Our research. jodrell bank centre for astrophysics
2013-03-20 ⚑r&d
pulsars , studying extreme physics, theories of gravity and the dynamic radio sky. Sun Planets Plasma and magnetic fields in the outer atmosphere of the Sun and the search for new planets orbiting other stars. Technology Including large.format imaging interferometric arrays, low.noise amplifiers and optical fibre data transfer. Feeds Disclaimer. Privacy. Copyright notice. Accessibility. Freedom of information Last updated Thursday
Welcome to the uk alma regional centre mdash; uk alma regional centre
pulsars , gravitational lensing, Planck and other CMB projects, dust and astrochemistry, star formation and evolution, and solar astronomy. There is also an active instrumentation group spanning the wavelength range from sub.mm to centimetre. In addition to ALMA and eMERLIN, observational interests include Herschel, the JCMT, the VLT and the VLTI. For more detail on our research please see JBCA Research. ALMA links ALMA Chile ESO
science.nrao.edu
Nrao science website mdash; science website
2012-02-07 ⚑tech
pulsars Astronomical Gifts That Keep on Giving Feb 17 , 2012 Vancouver, BC New Frontiers in the Radio Universe Feb 19 , 2012 Vancouver, BC 2nd EVLA Data Reduction Workshop Feb 22. Mar 01, 2012 Socorro, NM Outflows, Winds and Jets Workshop Mar 03. 06, 2012 Charlottesville, VA Tully.Fisher 35 Workshop Apr 01. 03, 2012 Green Bank, WV View Archived Events Staff. Policies. Diversity. Staff Login The National Radio Astronomy Observatory
Nrao image gallery
pulsars Neutron Stars 7 Black Holes 11 Planetary Nebulae 5 Galactic Center 14 Galactic Halo 17 Solar System 15 Sun 5 Planets 8 Moons 1 Asteroids 1 Comets 0 Miscellaneous 22 Astrochemistry 5 Protoplanetary Disks 2 Gamma.ray Bursters 1 Cosmology 6 Surveys 2 Image Compositions 6 Telescopes 154 GBT 34 VLA 63 VLBA 12 ALMA 40 12 m 2 140 ft 3 Other 0 ALMA Project 6 Science 0 Technology 2 Array Operations Site AOS 1 Operations Support
astro.fnal.gov
Fermilab center for particle astrophysics
2013-03-21 music
pulsars too faint to be detected individually, but perhaps collectively bright enough to make up this gamma.ray signal. This interpretation is a bit strained, however, by the degree of isotropy that is exhibited by the gamma.ray background. If enough bright pulsars were present far away from the Galactic Plane to make up the signal from the bubbles, then one would expect the gamma.ray background to be less isotropic than is
www.space.com
Seti and intelligent design
2014-11-09 shop
pulsars . stellar objects that flash light and radio waves into space with impressive regularity. pulsars were briefly tagged with the moniker LGM Little Green Men upon their discovery in 1967. Of course, these little men didn t have much to say. Regular pulses don t convey any information.no more than the ticking of a clock. But the real kicker is something else inefficiency. pulsars flash over the entire spectrum. No matter where
Welcome to the uk alma regional centre mdash; uk alma regional centre
pulsars , gravitational lensing, Planck and other CMB projects, dust and astrochemistry, star formation and evolution, and solar astronomy. There is also an active instrumentation group spanning the wavelength range from sub.mm to centimetre. In addition to ALMA and eMERLIN, observational interests include Herschel, the JCMT, the VLT and the VLTI. For more detail on our research please see JBCA Research. ALMA links ALMA Chile ESO
Nrao image gallery
pulsars Neutron Stars 7 Black Holes 11 Planetary Nebulae 5 Galactic Center 14 Galactic Halo 17 Solar System 15 Sun 5 Planets 8 Moons 1 Asteroids 1 Comets 0 Miscellaneous 22 Astrochemistry 5 Protoplanetary Disks 2 Gamma.ray Bursters 1 Cosmology 6 Surveys 2 Image Compositions 6 Telescopes 154 GBT 34 VLA 63 VLBA 12 ALMA 40 12 m 2 140 ft 3 Other 0 ALMA Project 6 Science 0 Technology 2 Array Operations Site AOS 1 Operations Support

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