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SRG/eROSITA discovery of a large circular SNR candidate G116.6−26.1: SN Ia explosion probing the gas of the Milky Way halo?
ABSTRACT We report a discovery of a new X-ray-selected supernova remnant (SNR) candidate SRGe J0023+3625 = G116.6−26.1 found in the SRG/eROSITA all-sky survey. The source features a large angular extent (∼4° in diameter), nearly circular shape, and X-ray spectrum dominated by emission lines of heliu...
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Published in: | Monthly notices of the Royal Astronomical Society 2021-10, Vol.507 (1), p.971-982 |
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creator | Churazov, E M Khabibullin, I I Bykov, A M Chugai, N N Sunyaev, R A Zinchenko, I I |
description | ABSTRACT
We report a discovery of a new X-ray-selected supernova remnant (SNR) candidate SRGe J0023+3625 = G116.6−26.1 found in the SRG/eROSITA all-sky survey. The source features a large angular extent (∼4° in diameter), nearly circular shape, and X-ray spectrum dominated by emission lines of helium- and hydrogen-like oxygen. It lacks bright counterparts of similar extent at other wavelengths which could be unequivocally associated with it. Given the relatively high Galactic latitude of the source, b ≈ −26°, we interpret these observational properties as an indication of the off-disc location of this SNR candidate. Namely, we propose that this object originated from a Type Ia supernotva which exploded some 40 000 yr ago in the low density ($\sim 10^{-3}\, {\rm cm^{-3}}$) and hot ($\sim (1{-}2)\times 10^6\, {\rm K}$) gas of the Milky Way halo at a distance of ∼3 kpc from the Sun. The low density of the halo gas implies that the cooling and collisional ionization equilibrium (CEI) time-scales downstream of the forward shock are much longer than the age of the SNR. This results in a relatively soft spectrum, reflecting pre-shock ionization state of the gas, and strong boost in the plasma emissivity (compared to CEI) due to enhanced collisional excitation through the increased electron temperature. If confirmed, such a rare object would provide us with a unique ‘in situ’ probe of physical conditions (density, temperature and metallicity) near the interface between the Milky Way’s disc and the halo. |
doi_str_mv | 10.1093/mnras/stab2125 |
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We report a discovery of a new X-ray-selected supernova remnant (SNR) candidate SRGe J0023+3625 = G116.6−26.1 found in the SRG/eROSITA all-sky survey. The source features a large angular extent (∼4° in diameter), nearly circular shape, and X-ray spectrum dominated by emission lines of helium- and hydrogen-like oxygen. It lacks bright counterparts of similar extent at other wavelengths which could be unequivocally associated with it. Given the relatively high Galactic latitude of the source, b ≈ −26°, we interpret these observational properties as an indication of the off-disc location of this SNR candidate. Namely, we propose that this object originated from a Type Ia supernotva which exploded some 40 000 yr ago in the low density ($\sim 10^{-3}\, {\rm cm^{-3}}$) and hot ($\sim (1{-}2)\times 10^6\, {\rm K}$) gas of the Milky Way halo at a distance of ∼3 kpc from the Sun. The low density of the halo gas implies that the cooling and collisional ionization equilibrium (CEI) time-scales downstream of the forward shock are much longer than the age of the SNR. This results in a relatively soft spectrum, reflecting pre-shock ionization state of the gas, and strong boost in the plasma emissivity (compared to CEI) due to enhanced collisional excitation through the increased electron temperature. If confirmed, such a rare object would provide us with a unique ‘in situ’ probe of physical conditions (density, temperature and metallicity) near the interface between the Milky Way’s disc and the halo.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stab2125</identifier><language>eng</language><publisher>London: Oxford University Press</publisher><subject>Density ; Electron energy ; Ionization ; Metallicity ; Sky surveys (astronomy) ; Supernova remnants ; X ray spectra ; X-ray astronomy</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2021-10, Vol.507 (1), p.971-982</ispartof><rights>2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society 2021</rights><rights>2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c341t-6244ae2d0a3fc5b1a5ee5c7e6a62b1537b08ea83b91e6017a6c0daf47fd4f2f63</citedby><cites>FETCH-LOGICAL-c341t-6244ae2d0a3fc5b1a5ee5c7e6a62b1537b08ea83b91e6017a6c0daf47fd4f2f63</cites><orcidid>0000-0003-2793-8229</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,1604,27924,27925</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/mnras/stab2125$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc></links><search><creatorcontrib>Churazov, E M</creatorcontrib><creatorcontrib>Khabibullin, I I</creatorcontrib><creatorcontrib>Bykov, A M</creatorcontrib><creatorcontrib>Chugai, N N</creatorcontrib><creatorcontrib>Sunyaev, R A</creatorcontrib><creatorcontrib>Zinchenko, I I</creatorcontrib><title>SRG/eROSITA discovery of a large circular SNR candidate G116.6−26.1: SN Ia explosion probing the gas of the Milky Way halo?</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
We report a discovery of a new X-ray-selected supernova remnant (SNR) candidate SRGe J0023+3625 = G116.6−26.1 found in the SRG/eROSITA all-sky survey. The source features a large angular extent (∼4° in diameter), nearly circular shape, and X-ray spectrum dominated by emission lines of helium- and hydrogen-like oxygen. It lacks bright counterparts of similar extent at other wavelengths which could be unequivocally associated with it. Given the relatively high Galactic latitude of the source, b ≈ −26°, we interpret these observational properties as an indication of the off-disc location of this SNR candidate. Namely, we propose that this object originated from a Type Ia supernotva which exploded some 40 000 yr ago in the low density ($\sim 10^{-3}\, {\rm cm^{-3}}$) and hot ($\sim (1{-}2)\times 10^6\, {\rm K}$) gas of the Milky Way halo at a distance of ∼3 kpc from the Sun. The low density of the halo gas implies that the cooling and collisional ionization equilibrium (CEI) time-scales downstream of the forward shock are much longer than the age of the SNR. This results in a relatively soft spectrum, reflecting pre-shock ionization state of the gas, and strong boost in the plasma emissivity (compared to CEI) due to enhanced collisional excitation through the increased electron temperature. If confirmed, such a rare object would provide us with a unique ‘in situ’ probe of physical conditions (density, temperature and metallicity) near the interface between the Milky Way’s disc and the halo.</description><subject>Density</subject><subject>Electron energy</subject><subject>Ionization</subject><subject>Metallicity</subject><subject>Sky surveys (astronomy)</subject><subject>Supernova remnants</subject><subject>X ray spectra</subject><subject>X-ray astronomy</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNqFkMFOwkAQhjdGExG9et7Ek4fCzm67BS-GEEUSlAQwHpvpdgvF0sXdYuzFs2efwGfxUXwSi-jZ0_zJ_P8_k4-QU2AtYF3RXhUWXduVGHPgwR5pgJCBx7tS7pMGYyLwOiHAITlybskY8wWXDfI6nQzaejKeDmc9mmROmWdtK2pSijRHO9dUZVZtakmndxOqsEiyBEtNBwCyJb_e3rlswUW9_PwYItUv69y4zBR0bU2cFXNaLjSdo9s2buVtlj9W9AErusDcXB6TgxRzp09-Z5PcX1_N-jfeaDwY9nsjTwkfSk9y30fNE4YiVUEMGGgdqFBLlDyGQIQx62jsiLgLWjIIUSqWYOqHaeKnPJWiSc52vfVbTxvtymhpNraoT0YCBDAu_BBqV2vnUtY4Z3UarW22QltFwKIt4-iHcfTHuA6c7wJms_7P-w2PHX9T</recordid><startdate>20211001</startdate><enddate>20211001</enddate><creator>Churazov, E M</creator><creator>Khabibullin, I I</creator><creator>Bykov, A M</creator><creator>Chugai, N N</creator><creator>Sunyaev, R A</creator><creator>Zinchenko, I I</creator><general>Oxford University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-2793-8229</orcidid></search><sort><creationdate>20211001</creationdate><title>SRG/eROSITA discovery of a large circular SNR candidate G116.6−26.1: SN Ia explosion probing the gas of the Milky Way halo?</title><author>Churazov, E M ; Khabibullin, I I ; Bykov, A M ; Chugai, N N ; Sunyaev, R A ; Zinchenko, I I</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c341t-6244ae2d0a3fc5b1a5ee5c7e6a62b1537b08ea83b91e6017a6c0daf47fd4f2f63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Density</topic><topic>Electron energy</topic><topic>Ionization</topic><topic>Metallicity</topic><topic>Sky surveys (astronomy)</topic><topic>Supernova remnants</topic><topic>X ray spectra</topic><topic>X-ray astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Churazov, E M</creatorcontrib><creatorcontrib>Khabibullin, I I</creatorcontrib><creatorcontrib>Bykov, A M</creatorcontrib><creatorcontrib>Chugai, N N</creatorcontrib><creatorcontrib>Sunyaev, R A</creatorcontrib><creatorcontrib>Zinchenko, I I</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Churazov, E M</au><au>Khabibullin, I I</au><au>Bykov, A M</au><au>Chugai, N N</au><au>Sunyaev, R A</au><au>Zinchenko, I I</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>SRG/eROSITA discovery of a large circular SNR candidate G116.6−26.1: SN Ia explosion probing the gas of the Milky Way halo?</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2021-10-01</date><risdate>2021</risdate><volume>507</volume><issue>1</issue><spage>971</spage><epage>982</epage><pages>971-982</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT
We report a discovery of a new X-ray-selected supernova remnant (SNR) candidate SRGe J0023+3625 = G116.6−26.1 found in the SRG/eROSITA all-sky survey. The source features a large angular extent (∼4° in diameter), nearly circular shape, and X-ray spectrum dominated by emission lines of helium- and hydrogen-like oxygen. It lacks bright counterparts of similar extent at other wavelengths which could be unequivocally associated with it. Given the relatively high Galactic latitude of the source, b ≈ −26°, we interpret these observational properties as an indication of the off-disc location of this SNR candidate. Namely, we propose that this object originated from a Type Ia supernotva which exploded some 40 000 yr ago in the low density ($\sim 10^{-3}\, {\rm cm^{-3}}$) and hot ($\sim (1{-}2)\times 10^6\, {\rm K}$) gas of the Milky Way halo at a distance of ∼3 kpc from the Sun. The low density of the halo gas implies that the cooling and collisional ionization equilibrium (CEI) time-scales downstream of the forward shock are much longer than the age of the SNR. This results in a relatively soft spectrum, reflecting pre-shock ionization state of the gas, and strong boost in the plasma emissivity (compared to CEI) due to enhanced collisional excitation through the increased electron temperature. If confirmed, such a rare object would provide us with a unique ‘in situ’ probe of physical conditions (density, temperature and metallicity) near the interface between the Milky Way’s disc and the halo.</abstract><cop>London</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/stab2125</doi><tpages>12</tpages><orcidid>https://orcid.org/0000-0003-2793-8229</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Density Electron energy Ionization Metallicity Sky surveys (astronomy) Supernova remnants X ray spectra X-ray astronomy |
title | SRG/eROSITA discovery of a large circular SNR candidate G116.6−26.1: SN Ia explosion probing the gas of the Milky Way halo? |
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