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Post-main-sequence planetary system evolution. [PDF]
R Soc Open Sci, 2016 Veras D.
europepmc +1 more source
Grand unification of neutron stars. [PDF]
Proc Natl Acad Sci U S A, 2010 Kaspi VM.
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Simulation-based Inference of Radio Millisecond Pulsars in Globular Clusters [PDF]
Joanna Berteaud +4 more
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Discovery and Timing of the First Millisecond Pulsar in NGC 6316
Deven Bhakta +3 more
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Nature, 1987
The recent discovery1,2 of a 3-millisecond pulsar in the globular cluster M28 (NGC6626) suggests that a few per cent of type I super novae (of which there are several subcategories, all associated with old stellar populations) form neutron stars. If the contact-binary white dwarf model for type Is is invoked3, it seems probable that millisecond pulsars
openaire +3 more sources
The recent discovery1,2 of a 3-millisecond pulsar in the globular cluster M28 (NGC6626) suggests that a few per cent of type I super novae (of which there are several subcategories, all associated with old stellar populations) form neutron stars. If the contact-binary white dwarf model for type Is is invoked3, it seems probable that millisecond pulsars
openaire +3 more sources
Nature Astronomy, 2021
Gamma-ray data from the Fermi Large Area Telescope reveal an unexplained, apparently diffuse, signal from the Galactic bulge1–3 that peaks near ~2 GeV with an approximately spherical4 intensity profile ∝ r−2.4 (refs.
Anuj Gautam +6 more
semanticscholar +1 more source
Gamma-ray data from the Fermi Large Area Telescope reveal an unexplained, apparently diffuse, signal from the Galactic bulge1–3 that peaks near ~2 GeV with an approximately spherical4 intensity profile ∝ r−2.4 (refs.
Anuj Gautam +6 more
semanticscholar +1 more source