Results 101 to 110 of about 15,098 (205)

Imaging and Spectral Fitting of Bright Gamma-Ray Sources with the COSI Balloon Payload

open access: yesThe Astrophysical Journal
The Compton Spectrometer and Imager balloon payload (COSI-Balloon) is a wide field-of-view Compton gamma-ray telescope that operates in the 0.2–5 MeV bandpass.
Jarred M. Roberts   +19 more
doaj   +1 more source

First Detection of Polarization in X-Rays for PSR B0540-69 and Its Nebula

open access: yesThe Astrophysical Journal
We report on X-ray polarization measurements of the extragalactic Crab-like PSR B0540-69 and its Pulsar Wind Nebula (PWN) in the Large Magellanic Cloud, using a ∼850 ks Imaging X-ray Polarimetry Explorer (IXPE) exposure. The PWN is unresolved by IXPE. No
Fei Xie   +103 more
doaj   +1 more source

ELEMENT DISTRIBUTIONS IN THE CRAB NEBULA [PDF]

open access: green, 2012
Timothy J. Satterfield   +4 more
openalex   +1 more source

Infrared-to-Ultraviolet Wavelength-dependent Variations Within the Pulse Profile Peaks of the Crab Nebula Pulsar [PDF]

open access: bronze, 1996
S. S. Eikenberry   +5 more
openalex   +1 more source

The N(2D) + CH2CHCN (Vinyl Cyanide) Reaction: A Combined Crossed Molecular Beam and Theoretical Study and Implications for the Atmosphere of Titan. [PDF]

open access: yesJ Phys Chem A, 2022
Vanuzzo G   +10 more
europepmc   +1 more source

A Cacophony of Echoes from Daily Monitoring of the Crab Pulsar at Jodrell Bank

open access: yesThe Astrophysical Journal
Using archival data from the 42-foot telescope at the Jodrell Bank Observatory, we produce daily stacks of aligned giant pulses for the Crab pulsar, to study changes to the daily profiles between 2012 April and 2016 December.
Thierry Serafin Nadeau   +5 more
doaj   +1 more source

Gamma radiation from the Crab nebula above 35 MeV [PDF]

open access: yes
Electromagnetic radiation from the Crab nebula were observed, showing that the Crab is unique among strong X-ray sources in that major component in the low energy range (1 to 10 KeV) shows little or no temporal variation.
Bignami, G. F.   +6 more
core   +1 more source

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