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Funding text: This work is part of the project 'Transient Astrophysical Objects' GINOP 2.3.2-15-2016-00033 of the National Research, Development and Innovation Office (NKFIH), Hungary, funded by the European Union.; Laszlo Molnar was supported by the Premium Postdoctoral Research Program of the Hungarian Academy of Sciences. The research leading to these results has received funding from the LP2018-7 Lendulet grant of the Hungarian Academy of Sciences.; Funding for the SDSS-IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org.0false2026-03-16T14:19:53.644+00002026-01-23T07:49:26.319+00002020-08-05T09:24:33.890+0000true10066055TurtóczkiTímea
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<div class="JournalArticle Publication short-list"> <div class="authors"> <span class="author-name" mtid="10083232"> <a href="/gui2/?type=authors&mode=browse&sel=10083232" target="_blank">Jäger, Zoltán Jr. ✉</a> </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10001530"> <a href="/gui2/?type=authors&mode=browse&sel=10001530" target="_blank">Vinkó, József</a> </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10026009"> <a href="/gui2/?type=authors&mode=browse&sel=10026009" target="_blank">Bíró, Barna I.</a> </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10009807"> <a href="/gui2/?type=authors&mode=browse&sel=10009807" target="_blank">Hegedüs, Tibor</a> </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10032717"> <a href="/gui2/?type=authors&mode=browse&sel=10032717" target="_blank">Borkovits, Tamás</a> </span> <span class="author-type"> </span> ; <span class="author-name" > Jäger, Zoltán Sr. </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10054959"> <a href="/gui2/?type=authors&mode=browse&sel=10054959" target="_blank">Nagy, Andrea P.</a> </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10017692"> <a href="/gui2/?type=authors&mode=browse&sel=10017692" target="_blank">Molnár, László</a> </span> <span class="author-type"> </span> ; <span class="author-name" mtid="10027559"> <a href="/gui2/?type=authors&mode=browse&sel=10027559" target="_blank">Kriskovics, Levente</a> </span> <span class="author-type"> </span> </div ><div class="title"><a href="/gui2/?mode=browse¶ms=publication;31395641" mtid="31395641" target="_blank">A low-luminosity core-collapse supernova very similar to SN 2005cs</a></div> <div class="pub-info"> <span class="journal-title">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</span> <span class="journal-volume">496</span> : <span class="journal-issue">3</span> <span class="page"> pp. 3725-3740. , 16 p. </span> <span class="year">(2020)</span> </div> <div class="pub-end"><div class="identifier-list"> <span class="identifiers"> <span class="id identifier oa_PAY" title=" Fizetős "> <a style="color:blue" title="10.1093/mnras/staa1743" target="_blank" href="https://doi.org/10.1093/mnras/staa1743"> DOI </a> </span> <span class="id identifier oa_none" title="none"> <a style="color:blue" title="000574919300071" target="_blank" href="https://www.webofscience.com/wos/woscc/full-record/000574919300071"> WoS </a> </span> <span class="id identifier oa_GREEN" title=" Green "> <a style="color:black" title="158303" target="_blank" href="http://real.mtak.hu/158303"> REAL </a> </span> <span class="id identifier oa_none" title="none"> <a style="color:blue" title="85101313843" target="_blank" href="http://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-85101313843"> Scopus </a> </span> <span class="id identifier oa_none" title="none"> <a style="color:blue" title="2020MNRAS.496.3725J luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature is still under debate. Such SNe are similar to SN 2005cs, a well-observed LL Type II-P event, having low expansion velocities, and small ejected 56Ni mass. We have analytic models to light curves of core-collapse SNe. This allows the estimation of the most important physical parameters, like the radius of the progenitor star, the mass of the ejected envelope, the mass of the radioactive nickel synthesized during the explosion, among others. PSN J17292918+7542390 has $R_0 = 91_{-70}^{+119} \times 10^{11} \, \text{cm}$ , $M_\text{ej} = 9.89_{-1.00}^{+2.10} \, \mathrm{ M}_{\odot }$ , $E_{\mbox{kin}} = 0.65_{-0.18}^{+0.19} \, \text{foe}$ , and $v_{\mbox{exp}} = 3332_{-347}^{+216}$ km s−1, for its progenitor radius, ejecta mass, kinetic energy, and expansion velocity, respectively. The initial nickel mass of the PSN J17292918+7542390 turned out to be $1.55_{-0.70" target="_blank" href="http://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3725J luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature is still under debate. Such SNe are similar to SN 2005cs, a well-observed LL Type II-P event, having low expansion velocities, and small ejected 56Ni mass. We have analytic models to light curves of core-collapse SNe. This allows the estimation of the most important physical parameters, like the radius of the progenitor star, the mass of the ejected envelope, the mass of the radioactive nickel synthesized during the explosion, among others. PSN J17292918+7542390 has $R_0 = 91_{-70}^{+119} \times 10^{11} \, \text{cm}$ , $M_\text{ej} = 9.89_{-1.00}^{+2.10} \, \mathrm{ M}_{\odot }$ , $E_{\mbox{kin}} = 0.65_{-0.18}^{+0.19} \, \text{foe}$ , and $v_{\mbox{exp}} = 3332_{-347}^{+216}$ km s−1, for its progenitor radius, ejecta mass, kinetic energy, and expansion velocity, respectively. The initial nickel mass of the PSN J17292918+7542390 turned out to be $1.55_{-0.70"> ADS </a> </span> <span class="id identifier oa_none" title="none"> <a style="color:blue" title="2020MNRAS.496.3725J" target="_blank" href="http://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3725J"> ADS </a> </span> <span class="id identifier oa_GREEN" title=" Green "> <a style="color:blue" title="2007.07650" target="_blank" href="http://arxiv.org/abs/2007.07650"> arXiv </a> </span> <span class="id identifier oa_GREEN" title=" Green "> <a style="color:blue" title="39118" target="_blank" href="http://publicatio.bibl.u-szeged.hu/39118"> SZTE Publicatio </a> </span> </span> </div> <div class="short-pub-prop-list"> <span class="deleted-record">Központi kezelésű</span> <span class="short-pub-mtid"> Közlemény:31395641 </span> <span class="status-holder"><span class="status-data status-VALIDATED"> Egyeztetett </span></span> <span class="pub-core">Forrás Idéző </span> <span class="pub-type">Folyóiratcikk (Szakcikk ) </span> <!-- && !record.category.scientific --> <span class="pub-category">Tudományos</span> <div class="publication-citation" style="margin-left: 0.5cm;"> <span title="Nyilvános idézőközlemények összesen, említések nélkül" class="citingPub-count">Nyilvános idéző összesen: 11</span> | Független: 11 | Függő: 0 | Nem jelölt: 0 | WoS jelölt: 10 | Scopus jelölt: 8 | WoS/Scopus jelölt: 10 | DOI jelölt: 10 </div> </div> </div> </div><div class="JournalArticle Publication long-list">
<div class="authors">
<img title="Forrásközlemény" style="float: left" src="/frontend/resources/grid/publication-core-icon.png">
<img title="Idézőközlemény" style="float: left" src="/frontend/resources/grid/publication-citation-icon.png">
<div class="autype autype0"> <span class="author-name" mtid="10083232"><a
href="/gui2/?type=authors&mode=browse&sel=10083232" target="_blank">Jäger Zoltán Jr. ✉
(<span class="authorship-author-name">Jäger Zoltán</span>
<span class="authorAux-mtmt"> Fizika, csillagászat</span>)
</a>
</span>
<span class="author-affil"><span title="Szegedi Tudományegyetem">SZTE</span>/Szegedi Tudományegyetem Bajai Obszervatóriuma</span>
;
<span class="author-name" mtid="10001530"><a
href="/gui2/?type=authors&mode=browse&sel=10001530" target="_blank">Vinkó József
(<span class="authorship-author-name">Vinkó József</span>
<span class="authorAux-mtmt"> Csillagászat asztrofizika</span>)
</a>
</span>
<span class="author-affil"><span title="Csillagászati és Földtudományi Kutatóközpont">CSFK</span>/Konkoly Thege Miklós Csillagászati Intézet; <span title="Szegedi Tudományegyetem">SZTE</span>/<span title="Természettudományi és Informatikai Kar">TTIK</span>/<span title="Fizikus Tanszékcsoport">FTCS</span>/Optikai és Kvantumelektronikai Tanszék</span>
;
<span class="author-name" mtid="10026009"><a
href="/gui2/?type=authors&mode=browse&sel=10026009" target="_blank">Bíró Barna I.
(<span class="authorship-author-name">Bíró Imre Barna</span>
<span class="authorAux-mtmt"> Csillagászat</span>)
</a>
</span>
<span class="author-affil"><span title="Szegedi Tudományegyetem">SZTE</span>/Szegedi Tudományegyetem Bajai Obszervatóriuma</span>
;
<span class="author-name" mtid="10009807"><a
href="/gui2/?type=authors&mode=browse&sel=10009807" target="_blank">Hegedüs Tibor
(<span class="authorship-author-name">Hegedüs Tibor</span>
<span class="authorAux-mtmt"> Asztrofizika</span>)
</a>
</span>
<span class="author-affil"><span title="Szegedi Tudományegyetem">SZTE</span>/Szegedi Tudományegyetem Bajai Obszervatóriuma</span>
;
<span class="author-name" mtid="10032717"><a
href="/gui2/?type=authors&mode=browse&sel=10032717" target="_blank">Borkovits Tamás
(<span class="authorship-author-name">Borkovits Tamás</span>
<span class="authorAux-mtmt"> Csillagászat</span>)
</a>
</span>
<span class="author-affil"><span title="Csillagászati és Földtudományi Kutatóközpont">CSFK</span>/Konkoly Thege Miklós Csillagászati Intézet; <span title="Szegedi Tudományegyetem">SZTE</span>/Szegedi Tudományegyetem Bajai Obszervatóriuma</span>
;
<span class="author-name" >Jäger Zoltán Sr.
</span>
;
<span class="author-name" mtid="10054959"><a
href="/gui2/?type=authors&mode=browse&sel=10054959" target="_blank">Nagy Andrea P.
(<span class="authorship-author-name">Nagy Andrea</span>
<span class="authorAux-mtmt"> Asztrofizika</span>)
</a>
</span>
<span class="author-affil"><span title="Csillagászati és Földtudományi Kutatóközpont">CSFK</span>/Konkoly Thege Miklós Csillagászati Intézet; <span title="Szegedi Tudományegyetem">SZTE</span>/<span title="Természettudományi és Informatikai Kar">TTIK</span>/<span title="Fizikai Intézet">FI</span>/Optikai és Kvantumelektronikai Tanszék</span>
;
<span class="author-name" mtid="10017692"><a
href="/gui2/?type=authors&mode=browse&sel=10017692" target="_blank">Molnár László
(<span class="authorship-author-name">Molnár László</span>
<span class="authorAux-mtmt"> Csillagászat</span>)
</a>
</span>
<span class="author-affil"><span title="Csillagászati és Földtudományi Kutatóközpont">CSFK</span>/Konkoly Thege Miklós Csillagászati Intézet; <span title="Eötvös Loránd Tudományegyetem">ELTE</span>/<span title="Természettudományi Kar">TTK</span>/Fizikai Intézet; <span title="Csillagászati és Földtudományi Kutatóközpont">CSFK</span>/<span title="Konkoly Thege Miklós Csillagászati Intézet">CSKI</span>/MTA CSFK Lendület Lokális Kozmológia Kutatócsoport</span>
;
<span class="author-name" mtid="10027559"><a
href="/gui2/?type=authors&mode=browse&sel=10027559" target="_blank">Kriskovics Levente
(<span class="authorship-author-name">Kriskovics Levente</span>
<span class="authorAux-mtmt"> Csillagaktivitás</span>)
</a>
</span>
<span class="author-affil"><span title="Csillagászati és Földtudományi Kutatóközpont">CSFK</span>/Konkoly Thege Miklós Csillagászati Intézet; <span title="Eötvös Loránd Tudományegyetem">ELTE</span>/<span title="Természettudományi Kar">TTK</span>/Fizikai Intézet</span>
</div>
</div>
<div class="title"><a href="/gui2/?mode=browse¶ms=publication;31395641" target="_blank">A low-luminosity core-collapse supernova very similar to SN 2005cs</a></div> <div> <span class="journal-title">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</span>
<span class="journal-issn">(<a target="_blank" href="https://portal.issn.org/resource/ISSN/0035-8711">0035-8711</a> <a target="_blank" href="https://portal.issn.org/resource/ISSN/1365-2966">1365-2966</a>)</span>:
<span class="journal-volume">496</span> <span class="journal-issue">3</span>
<span class="page">
pp 3725-3740
</span> <span class="year">(2020)</span>
</div>
<div class="pub-footer">
<span class="language" xmlns="http://www.w3.org/1999/html">Nyelv:
Angol
| </span>
<span class="identifiers">
<span class="id identifier oa_PAY" title=" Fizetős
">
<a style="color:blue" title="10.1093/mnras/staa1743" target="_blank" href="https://doi.org/10.1093/mnras/staa1743">
DOI
</a>
</span>
<span class="id identifier oa_none" title="none">
<a style="color:blue" title="000574919300071" target="_blank" href="https://www.webofscience.com/wos/woscc/full-record/000574919300071">
WoS
</a>
</span>
<span class="id identifier oa_GREEN" title=" Green
">
<a style="color:black" title="158303" target="_blank" href="http://real.mtak.hu/158303">
REAL
</a>
</span>
<span class="id identifier oa_none" title="none">
<a style="color:blue" title="85101313843" target="_blank" href="http://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-85101313843">
Scopus
</a>
</span>
<span class="id identifier oa_none" title="none">
<a style="color:blue" title="2020MNRAS.496.3725J luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature is still under debate. Such SNe are similar to SN 2005cs, a well-observed LL Type II-P event, having low expansion velocities, and small ejected 56Ni mass. We have analytic models to light curves of core-collapse SNe. This allows the estimation of the most important physical parameters, like the radius of the progenitor star, the mass of the ejected envelope, the mass of the radioactive nickel synthesized during the explosion, among others. PSN J17292918+7542390 has $R_0 = 91_{-70}^{+119} \times 10^{11} \, \text{cm}$ , $M_\text{ej} = 9.89_{-1.00}^{+2.10} \, \mathrm{ M}_{\odot }$ , $E_{\mbox{kin}} = 0.65_{-0.18}^{+0.19} \, \text{foe}$ , and $v_{\mbox{exp}} = 3332_{-347}^{+216}$ km s−1, for its progenitor radius, ejecta mass, kinetic energy, and expansion velocity, respectively. The initial nickel mass of the PSN J17292918+7542390 turned out to be $1.55_{-0.70" target="_blank" href="http://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3725J luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature is still under debate. Such SNe are similar to SN 2005cs, a well-observed LL Type II-P event, having low expansion velocities, and small ejected 56Ni mass. We have analytic models to light curves of core-collapse SNe. This allows the estimation of the most important physical parameters, like the radius of the progenitor star, the mass of the ejected envelope, the mass of the radioactive nickel synthesized during the explosion, among others. PSN J17292918+7542390 has $R_0 = 91_{-70}^{+119} \times 10^{11} \, \text{cm}$ , $M_\text{ej} = 9.89_{-1.00}^{+2.10} \, \mathrm{ M}_{\odot }$ , $E_{\mbox{kin}} = 0.65_{-0.18}^{+0.19} \, \text{foe}$ , and $v_{\mbox{exp}} = 3332_{-347}^{+216}$ km s−1, for its progenitor radius, ejecta mass, kinetic energy, and expansion velocity, respectively. The initial nickel mass of the PSN J17292918+7542390 turned out to be $1.55_{-0.70">
ADS
</a>
</span>
<span class="id identifier oa_none" title="none">
<a style="color:blue" title="2020MNRAS.496.3725J" target="_blank" href="http://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3725J">
ADS
</a>
</span>
<span class="id identifier oa_GREEN" title=" Green
">
<a style="color:blue" title="2007.07650" target="_blank" href="http://arxiv.org/abs/2007.07650">
arXiv
</a>
</span>
<span class="id identifier oa_GREEN" title=" Green
">
<a style="color:blue" title="39118" target="_blank" href="http://publicatio.bibl.u-szeged.hu/39118">
SZTE Publicatio
</a>
</span>
</span>
<OnlyViewableByAuthor><div class="ratings">
<div class="journal-subject">Folyóirat szakterülete: Scopus - Astronomy and Astrophysics SJR indikátor: Q1</div>
<div class="journal-subject">Folyóirat szakterülete: Scopus - Space and Planetary Science SJR indikátor: Q1</div>
</div></OnlyViewableByAuthor>
<div class="publication-citation" style="margin-left: 0.5cm;">
<span title="Nyilvános idézőközlemények összesen, említések nélkül" class="citingPub-count">Nyilvános idéző összesen: 11</span>
| Független: 11
| Függő: 0
| Nem jelölt: 0
| WoS jelölt: 10
| Scopus jelölt: 8
| WoS/Scopus jelölt: 10
| DOI jelölt: 10
</div>
<div class="publication-citation">
<a target="_blank" href="/api/publication?cond=citations.related;eq;31395641&sort=publishedYear,desc&sort=title">
Idézett közlemények száma: 6
</a>
</div>
<div class="mtid"><span class="long-pub-mtid">Közlemény: 31395641</span>
| <span class="status-data status-VALIDATED"> Egyeztetett
</span>
Forrás Idéző
| <span class="type-subtype">Folyóiratcikk
( Szakcikk
)
</span>
| <span class="pub-category">Tudományos</span>
| <span class="publication-sourceOfData">RIS-ADS</span>
</div>
<div class="lastModified">Utolsó módosítás: 2026.01.23. 08:49 Vasvari Lilian (MTMT Központ, admin)
</div>
<div class="lockedBy">Központi kezelésű 2023.07.24. 15:11 Pécsi Éva (MTMT Közp 2,3, admin)
</div>
<pre class="comment" style="margin-top: 0; margin-bottom: 0;"><u>Megjegyzés</u>: Funding Agency and Grant Number: European Union [GINOP 2.3.2-15-2016-00033]; Premium Postdoctoral Research Program of the Hungarian Academy of Sciences; Lendulet grant of the Hungarian Academy of Sciences [LP2018-7]; Alfred P. Sloan Foundation; U.S. Department of Energy Office of Science; Center for High-Performance Computing at the University of Utah
Funding text: This work is part...</pre>
</div></div>