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- Open Position: Research Intern06 Aug, 2020
- Recorded Session: Arecibo Observatory Virtual Town Hall30 Jul, 2020
- The Arecibo Observatory congratulates Dr. Martha P. Haynes, recipient of the Janksy Lectureship 2020! 23 Jul, 2020
- AO Adapts: Continued Workshops, Training, and Education06 Jul, 2020
- Annoucing the Arecibo Observatory Town Hall01 Jul, 2020
- AO Features: Former AO Postdoctoral Researcher Kristen Jones30 Jun, 2020
- New AO Lidar Observations of Ca+ in the Mesosphere and Thermosphere29 Jun, 2020
- Breaking Assumptions on the Excitation Temperatures in Molecular Clouds29 Jun, 2020
- Modifying the Earth’s Ionosphere from Arecibo29 Jun, 2020
- AO radar measurements of Jupiter’s Moons29 Jun, 2020
- A New Approach for Understanding the Occurrence Rate of MSTIDs in the Caribbean Nighttime Ionosphere29 Jun, 2020
- Asteroid Visiting Earth’s Neighborhood Brings its Own Face Mask 23 Apr, 2020
- REU Students’ Research & Presentations01 Apr, 2020
- Transforming the Arecibo Observatory into a Classroom31 Mar, 2020
- Arecibo Observatory re-enters VLBI network with 21st-century backend31 Mar, 2020
Artistic impression of the cosmic cow. Credit: Shanghai Astronomical Observatory, China.
|Astronomy||AO helps detect Magnetar in the Cow|
The Arecibo Observatory was one of 21 telescopes involved in the large-scale European Very Large Baseline Interferometry (VLBI) Network (EVN) radio observations of the astronomical explosion AT2018cow ('the Cow'). AO, which has the largest collecting area of all of the participating telescopes, helped boost the sensitivity of the extended VLBI baselines to detect the radio signals, producing high-resolution images that enabled scientists to determine that the highly unique supernova resulted in the creation of a magnetar – a neutron star with a very strong magnetic field.
AT2018cow was initially detected on June 16, 2018 by the NASA-funded ATLAS-HKO telescope, located at the Haleakala Observatory in Hawaii and was over 10 times brighter than a typical supernova and approximately 8 times as bright as its host galaxy. The event occurred about 200 million lightyears away in the star-forming region CGCG 137-068, in the constellation Hercules.
This particular supernova caught the interest of the astronomical community because the event remained bright with a relatively constant spectrum at x-ray and UV wavelengths for nearly 3 weeks, which is unusual for a supernova. This indicated that there was likely a central engine at the core of the event, driving the explosion. Some attributed the powerful event to the tidal disruption of a star by an intermediate mass black hole, while others suggested that the core of the supernova had collapsed inward.
The explanation for the central engine was debated until the recent VLBI study, led by Dr. Prashanth Mohan, which consisted of 5 VLBI sessions lasting approximately one year. Arecibo observatory participated in the second VLBI session for the 5 GHz campaign, contributing about 4 hours of data.
From the follow-up VLBI observations, the team found that there were no relativistic jets, meaning that a supernova was a better explanation for AT2018cow. Of particular interest was how the radio signals faded from the central engine, which suggested that the supernova explosion had expanded into a dense, magnetized environment. This led the scientists to conclude that the central engine of AT2018cow is a magnetar.
Article written by Dr. Tracy Becker - AO Collaborator / SwRI Research Scientist
Head of the Astronomy Dept.
Keywords: arecibo, observatory, cow, vlvi, at2018cow, magnetar, telescope, radio, astronomical, CGCG, EVN, NASA, ATLAS-HKO, supernova