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The Matter Beyond the Ring: The Recent Evolution of SN 1987A Observed by the Hubble Space Telescope
KTH, School of Biotechnology (BIO), Centres, Albanova VinnExcellence Center for Protein Technology, ProNova. KTH, School of Engineering Sciences (SCI), Physics. (Oskar Klein Ctr)
Stockholm Univ, Dept Astron, AlbaNova, Oskar Klein Ctr, SE-10691 Stockholm, Sweden..
KTH, School of Engineering Sciences (SCI), Physics. KTH, School of Biotechnology (BIO), Centres, Albanova VinnExcellence Center for Protein Technology, ProNova. (Oskar Klein Ctr)
Harvard Smithsonian Ctr Astrophys, 60 Garden St,MS-19, Cambridge, MA 02138 USA..
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2019 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 886, no 2, article id 147Article in journal (Refereed) Published
Abstract [en]

The nearby SN 1987A offers a spatially resolved view of the evolution of a young supernova (SN) remnant. Here we present recent Hubble Space Telescope imaging observations of SN 1987A, which we use to study the evolution of the ejecta, the circumstellar equatorial ring (ER), and the increasing emission from material outside the ER. We find that the inner ejecta have been brightening at a gradually slower rate and that the western side has been brighter than the eastern side since similar to 7000 days. This is expected given that the X-rays from the ER are most likely powering the ejecta emission. At the same time, the optical emission from the ER continues to fade linearly with time. The ER is expanding at 680 50 km s(-1), which reflects the typical velocity of transmitted shocks in the dense hot spots. A dozen spots and a rim of diffuse H alpha emission have appeared outside the ER since 9500 days. The new spots are more than an order of magnitude fainter than the spots in the ER and also fade faster. We show that the spots and diffuse emission outside the ER may be explained by fast ejecta interacting with high-latitude material that extends from the ER toward the outer rings. Further observations of this emission will make it possible to determine the detailed geometry of the high-latitude material and provide insight into the formation of the rings and the mass-loss history of the progenitor.

Place, publisher, year, edition, pages
IOP PUBLISHING LTD , 2019. Vol. 886, no 2, article id 147
Keywords [en]
Core-collapse supernovae, Supernova remnants, Circumstellar matter, Shocks, Ejecta
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-266280DOI: 10.3847/1538-4357/ab4ff2ISI: 000501188000001OAI: oai:DiVA.org:kth-266280DiVA, id: diva2:1383552
Note

QC 20200108

Available from: 2020-01-08 Created: 2020-01-08 Last updated: 2020-01-08Bibliographically approved

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