On the origin of the asymmetry of the ejecta structure and explosion of G350.1−0.3

Simple item page
dc.contributor.authorTsuchioka, Tomoya
dc.contributor.authorUchiyama, Yasunobu
dc.contributor.authorHigurashi, Ryota
dc.contributor.authorIwasaki, Hiroyoshi
dc.contributor.authorOtsuka, Shumpei
dc.contributor.authorYamada, Shinya
dc.contributor.authorSato, Toshiki
dc.date.accessioned2021-05-03T17:19:16Z
dc.date.available2021-05-03T17:19:16Z
dc.description.abstractWe present X-ray analysis of the ejecta of supernova remnant G350.1−0.3 observed with Chandra and Suzaku, and clarify the ejecta's kinematics over a decade and obtain a new observational clue to understanding the origin of the asymmetric explosion. Two images of Chandra X-ray Observatory taken in 2009 and 2018 are analyzed in several methods, and enable us to measure the velocities in the plane of the sky. A maximum velocity is 4640±290 km s⁻¹ (0.218±0.014 arcsec yr⁻¹) in the eastern region in the remnant. These findings trigger us to scrutinize the Doppler effects in the spectra of the thermal emission, and the velocities in the line-of-sight direction are estimated to be a thousand km s⁻1. The results are confirmed by analyzing the spectra of Suzaku. Combining the proper motions and line-of-sight velocities, the ejecta's three-dimensional velocities are ∼3000-5000 km s⁻¹. The center of the explosion is more stringently constrained by finding the optimal time to reproduce the observed spatial expansion. Our findings that the age of the SNR is estimated at most to be 655 years, and the CCO is observed as a point source object against the SNR strengthen the 'hydrodynamical kick' hypothesis on the origin of the remnant.en_US
dc.description.sponsorshipThis work was supported by JSPS KAKENHI Grant Numbers 18H03722, 20H01941, and 20K20527.en_US
dc.description.urihttps://arxiv.org/abs/2104.03001en_US
dc.format.extent12 pagesen_US
dc.genrejournal articles preprintsen_US
dc.identifierdoi:10.13016/m2fhp0-ffsx
dc.identifier.citationTomoya Tsuchioka, Yasunobu Uchiyama, Ryota Higurashi, Hiroyoshi Iwasaki, Shumpei Otsuka, Shinya Yamada and Toshiki Sato, On the origin of the asymmetry of the ejecta structure and explosion of G350.1−0.3, https://arxiv.org/abs/2104.03001en_US
dc.identifier.urihttp://hdl.handle.net/11603/21430
dc.language.isoen_USen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsAttribution 4.0 International*
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/*
dc.titleOn the origin of the asymmetry of the ejecta structure and explosion of G350.1−0.3en_US
dc.typeTexten_US

Files

Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
2104.03001.pdf
Size:
4.93 MB
Format:
Adobe Portable Document Format
Description:
Download
License bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
2.56 KB
Format:
Item-specific license agreed upon to submission
Description:
Download

Collections

UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
UMBC Faculty Collection