Tag Archive for 'Vela pulsar'

This DECam image shows the Vela supernova remnant, a remnant of supernova explosion located 800 light-years away in the southern constellation of Vela. Image credit: CTIO / NOIRLab / DOE / NSF / AURA / T.A. Rector, University of Alaska Anchorage & NSF’s NOIRLab / M. Zamani & D. de Martin, NSF’s NOIRLab.

Dark Energy Camera Captures Gigapixel Image of Vela Supernova Remnant

Mar 12, 2024 by News Staff

Astronomers using the powerful Dark Energy Camera (DECam) on the Víctor M. Blanco 4-m telescope at Cerro Tololo Inter-American Observatory, a Program...

This image shows the Vela pulsar wind nebula: light blue represents X-ray polarization data from IXPE; pink and purple colors correspond to data from NASA’s Chandra X-ray observatory; the NASA/ESA Hubble Space Telescope contributed the stars in the background. Image credit: IXPE / NASA / MSFC / Fei Xie / CXC / SAO / STScI / Hubble / Chandra / Judy Schmidt / Kimberly Arcand / Nancy Wolk.

Polarized X-ray Detection Sheds New Light on Vela Pulsar Wind Nebula

Mar 8, 2023 by News Staff

Astronomers using the Imaging X-ray Polarimetry Explorer (IXPE) — a collaboration between NASA and the Italian Space Agency — have observed...

This image, taken by the OmegaCAM camera at ESO’s VLT Survey Telescope, shows a spectacular view of the orange and pink clouds that make up the Vela SNR. OmegaCAM can take images through several filters that let through light of different colors. In this particular image of the Vela SNR, four different filters were used, represented here by a combination of magenta, blue, green and red. Image credit: ESO / VPHAS+ Team / Cambridge Astronomical Survey Unit.

OmegaCAM Snaps Beautiful Image of Vela Supernova Remnant

Nov 1, 2022 by Enrico de Lazaro

Astronomers using the 268-million-pixel OmegaCAM instrument on ESO’s VLT Survey Telescope have captured a detailed image of the Vela supernova remnant,...

Glitch in Vela Pulsar Provides Unique Opportunity to Study Neutron Star’s Interior

Aug 13, 2019 by News Staff

Pulsars are rapidly rotating neutron stars observed to have pulses of radiation at very regular intervals that typically range from milliseconds to seconds....