Results 11 to 20 of about 99,264 (157)

Supernova Cosmology: Legacy and Future [PDF]

open access: yes, 2011
The discovery of dark energy by the first generation of high-redshift supernova surveys has generated enormous interest beyond cosmology and has dramatic implications for fundamental physics.
A. Goobar, B. Leibundgut
semanticscholar   +3 more sources

A Pre-Gaia Census of Nearby Stellar Groups [PDF]

open access: yesProceedings of the International Astronomical Union, 2015
The nearest, youngest groups of stars to the Sun provide important samples of age-dated stars for studying circumstellar disk evolution, imaged exoplanets, and brown dwarfs. I briefly comment on the status of the known stellar groups within 100 pc: β Pic,
E. Mamajek
semanticscholar   +3 more sources

Possibility of Secondary i- and s-processes Following r-process in the Collapsar Jet

open access: yesThe Astrophysical Journal Letters
The slow and intermediate neutron-capture processes, s - and i -processes, are believed to occur in asymptotic giant branch stars to provide half of the heavy atomic nuclei with A ≥ 90. We suggest a possibility that certain types of outflows found in the
Zhenyu He   +7 more
doaj   +2 more sources

NEOWISE-R Caught the Luminous SN 2023ixf in Messier 101 [PDF]

open access: yesThe Astrophysical Journal
During routine survey imaging, the reactivated Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE-R) serendipitously caught the Type II supernova SN 2023ixf in Messier 101 on the rise, starting day 3.6 through day 10.9, and again on the ...
Schuyler D. Van Dyk   +18 more
doaj   +2 more sources

Inference of bipolar neutrino flavor oscillations near a core-collapse supernova based on multiple measurements at Earth [PDF]

open access: bronzePhysical Review D, 2022
Neutrinos in compact-object environments, such as core-collapse supernovae, can experience various kinds of collective effects in flavor space, engendered by neutrino-neutrino interactions.
Eve Armstrong   +6 more
openalex   +3 more sources

Is the PAMELA anomaly caused by supernova explosions near the Earth? [PDF]

open access: green, 2009
We show that the anomaly of the positron fraction observed by the PAMELA experiment can be attributed to recent supernova explosion(s) in a dense gas cloud near the Earth. Protons are accelerated around the supernova remnant.
Yutaka Fujita   +3 more
openalex   +3 more sources

Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. II. Advanced modelling of interstellar 26Al, 53Mn, 60Fe, and 244Pu influxes as traces of past supernova activity in the solar neighbourhood [PDF]

open access: yesAstronomy & Astrophysics, 2023
Measurements of long-lived radioisotopes provide a means, completely independent of other observational channels, to draw conclusions about near-Earth supernovae (SNe) and thus the origin of the Local Bubble (LB).
M. Schulreich   +2 more
semanticscholar   +1 more source

Photons from Neutrinos: The Gamma-Ray Echo of a Supernova Neutrino Burst [PDF]

open access: yesAstrophysical Journal, 2023
When a star undergoes core collapse, a vast amount of energy is released in a ∼10 s long burst of neutrinos of all species. Inverse beta decay in the star’s hydrogen envelope causes an electromagnetic cascade that ultimately results in a flare of gamma ...
C. Lunardini   +5 more
semanticscholar   +1 more source

Particle acceleration in winds of star clusters [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
The origin of cosmic rays in our Galaxy remains a subject of active debate. While supernova remnant (SNR) shocks are often invoked as the sites of acceleration, it is now widely accepted that the difficulties of such sources in reaching PeV energies ...
G. Morlino   +3 more
semanticscholar   +1 more source

The Thousand-Pulsar-Array programme on MeerKAT - X. Scintillation arcs of 107 pulsars [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
We present the detection of 107 pulsars with interstellar scintillation arcs at 856–1712 MHz, observed with the MeerKAT Thousand Pulsar Array Programme.
R. Main   +11 more
semanticscholar   +1 more source

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