Results 101 to 110 of about 76,238 (239)
Cherenkov Telescope Array Observatory: Die Zukunft der Gammaastronomie
Im Jahr 1989 hat das Wipple‐Observatorium die erste Quelle hochenergetischer Gammastrahlung entdeckt. 2002 waren dann sechs Quellen bekannt, 2024 schon mehr als 300. Und das ist immer noch lediglich die Spitze des Eisbergs in der jungen Geschichte der Gammaastronomie.
Daniela Hadasch, Daniel Mazin
wiley +1 more source
ASKAP Detection of the Ultra-Long Spin Period Pulsar PSR J0901-4046
A radio source with a period of 75.88 s, suspected of being an ultra-long period pulsar, was discovered in 2020 with the MeerKAT radio telescope.
Emil Lenc +3 more
doaj +1 more source
Twenty Years of Searching for (and Finding) Globular Cluster Pulsars
Globular clusters produce orders of magnitude more millisecond pulsars per unit mass than the Galactic disk. Since the first cluster pulsar was uncovered twenty years ago, at least 138 have been identified - most of which are binary millisecond pulsars ...
A. Cumming +4 more
core +1 more source
Probing the solar interior with lensed gravitational waves from known pulsars [PDF]
Ryuichi Takahashi +2 more
openalex +1 more source
Effects of Spin Properties on Braking Indices of 208 Glitching Pulsars [PDF]
Juliana Nwakaego Odo +1 more
openalex +1 more source
Alfvén Wave Mode Conversion in Pulsar Magnetospheres [PDF]
Yajie Yuan +3 more
openalex +1 more source
X‐Ray Emission from the Planet Pulsar B1257+12 [PDF]
G. G. Pavlov +3 more
openalex +1 more source
E. ASSÉO, D. BEAUFILS, R. PELLAT
openaire +1 more source
SYSTEMATIC AND STOCHASTIC VARIATIONS IN PULSAR DISPERSION MEASURES [PDF]
M. T. Lam +5 more
openalex +1 more source
Pulsar timing arrays (PTAs) are designed to detect nanohertz-frequency gravitational waves (GWs). Since GWs are anticipated from cosmic strings, PTAs offer a viable approach to testing their existence.
Yong Xia +13 more
doaj +1 more source

