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Correction to: Modelling annual scintillation velocity variations of FRBĀ 20201124A.
- Source :
-
Monthly Notices of the Royal Astronomical Society: Letters . Oct2023, Vol. 525 Issue 1, pL28-L28. 1p. - Publication Year :
- 2023
-
Abstract
- This document is a correction notice for an article titled "Modelling Annual Scintillation Velocity Variations of FRB 20201124A" published in the Monthly Notices of the Royal Astronomical Society: Letters. The correction addresses a typo in the published abstract, where "pc" should be replaced by "kpc." The corrected abstract discusses the measurement of scintillation velocity at 10 epochs over a year, indicating that the screen is within the Milky Way. The modeling of the annual variation suggests a screen distance of 0.40±0.04 kpc or 0.46±0.06 kpc from Earth, potentially associated with material outside of the Local Bubble or the edge of the Orion-Eridanus Superbubble. The authors of the article are R A Main, S Bethapudi, V R Marthi, M L Bause, D Z Li, H-H Lin, L G Spitler, and R S Wharton. [Extracted from the article]
- Subjects :
- *VELOCITY
*MILKY Way
Subjects
Details
- Language :
- English
- ISSN :
- 17453925
- Volume :
- 525
- Issue :
- 1
- Database :
- Academic Search Index
- Journal :
- Monthly Notices of the Royal Astronomical Society: Letters
- Publication Type :
- Academic Journal
- Accession number :
- 169973838
- Full Text :
- https://doi.org/10.1093/mnrasl/slad090