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The Astrophysical Journal, ISSN 0004-637X, 12/2008, Volume 689, Issue 2, pp. 1127 - 1140
Journal Article
Nature, ISSN 0028-0836, 05/2018, Volume 557, Issue 7706, pp. 522 - 525
Radio pulsars scintillate because their emission travels through the ionized interstellar medium along multiple paths, which interfere with each other. It has... 
FAST RADIO-BURST | MILLISECOND PULSAR | MULTIDISCIPLINARY SCIENCES | FRB 121102 | ASTROMETRY | MECHANISMS | HOST GALAXY | Observations | Stars, Double | Pulsars | Supernova | Plasma | Radio bursts | Variations | Density | Emissions | Supernova remnants | Outflow | Emissions control | Interstellar medium | Companion stars | Electric fields | Interstellar matter | Lenses | Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 06/2015, Volume 806, Issue 1, pp. L1 - 5
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 05/2017, Volume 840, Issue 2, p. L15
Journal Article
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, ISSN 1364-503X, 06/2013, Volume 371, Issue 1992, p. 20120236
Thermonuclear supernovae result when interaction with a companion reignites nuclear fusion in a carbon-oxygen white dwarf, causing a thermonuclear runaway, a... 
Supernovae: general | Binaries: close | White dwarfs | PROGENITORS | IA SUPERNOVAE | MULTIDISCIPLINARY SCIENCES | CIRCUMSTELLAR MATERIAL | binaries: close | supernovae: general | MASS MODELS | SUB-CHANDRASEKHAR SUPERNOVAE | DELAY-TIME DISTRIBUTION | white dwarfs | EVOLUTION | BINARIES | ASYMMETRIC EXPLOSION | DETONATION | Physics - High Energy Astrophysical Phenomena
Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 10/2010, Volume 722, Issue 2, pp. L157 - L161
Type Ia supernovae (SNe Ia) are generally thought to be due to the thermonuclear explosions of carbon-oxygen white dwarfs (COWDs) with masses near the... 
Supernovae: general | Binaries: close | White dwarfs | binaries: close | EXPLOSION | CLOSE BINARIES | supernovae: general | HYDROGEN | white dwarfs | EVOLUTION | MODELS | ASTRONOMY & ASTROPHYSICS | MASS | FACTORY OBSERVATIONS | CONSTRAINTS | SPECTRUM | DETONATIONS | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2013, Volume 767, Issue 2, pp. 164 - 32
Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 10/2011, Volume 740, Issue 1, p. L30
We present a phase-coherent timing solution for RX J0420.0-5022, the coolest (kT similar or equal to 45 eV) and fastest-spinning (P = 3.45 s) of the seven... 
stars: individual (RX J0420.0-5022) | stars: neutron | X-rays: stars | POPULATION | MAGNETIC-FIELDS | SPIN-DOWN | ASTRONOMY & ASTROPHYSICS | X-RAY | EMISSION | Physics - High Energy Astrophysical Phenomena | MAGNETIC FIELDS | MULTIPOLES | MATHEMATICAL SOLUTIONS | DIPOLES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NEUTRON STARS | STARS
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 11/2018, Volume 867, Issue 1, p. L2
Many radio pulsars have stable pulse profiles, but some exhibit mode changing where the profile switches between two or more quasi-stable modes of emission. So... 
radiation mechanisms: non-thermal | pulsars: individual (PSR B1957+20) | pulsars: general | ASTRONOMY & ASTROPHYSICS | DRIFTING SUBPULSES | B1937+21 | EMISSION | MODULATION | SINGLE-PULSE | Radio emission | Energy distribution | Switches | Pulsars | Emissions | Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal, ISSN 0004-637X, 2008, Volume 689, Issue 2, pp. L153 - L156
Journal Article