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Article: New Hubble Space Telescope observations of high-velocity Lyα and Hα in SNR 1987A
Title | New Hubble Space Telescope observations of high-velocity Lyα and Hα in SNR 1987A |
---|---|
Authors | |
Keywords | Circumstellar Matter Shocks Supernova Remnants |
Issue Date | 1998 |
Publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 |
Citation | Astrophysical Journal Letters, 1998, v. 509 n. 2 PART 2, p. L117-L120 How to Cite? |
Abstract | We describe and model high-velocity (≈15,000 km s -1) Lyα and Hα emission from the supernova remnant SNR 1987A seen in 1997 September and October with the Space Telescope Imaging Spectrograph. Part of this emission comes from a reverse shock located at ≈75% of the radius of the inner boundary of the inner circumstellar ring and confined within ± 30° of the equatorial plane. Departure from axisymmetry in the Lyα and Hα emission correlates with that seen in nonthermal radio emission and reveals an asymmetry in the circumstellar gas distribution. We also see diffuse high-velocity Lyα emission from supernova debris inside the reverse shock that may be due to excitation by nonthermal particles accelerated by the shock. |
Persistent Identifier | http://hdl.handle.net/10722/175105 |
ISSN | 2023 Impact Factor: 8.8 2023 SCImago Journal Rankings: 2.766 |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Michael, E | en_US |
dc.contributor.author | Mccray, R | en_US |
dc.contributor.author | Pun, CSJ | en_US |
dc.contributor.author | Borkowski, K | en_US |
dc.contributor.author | Garnavich, P | en_US |
dc.contributor.author | Challis, P | en_US |
dc.contributor.author | Kirshner, RP | en_US |
dc.contributor.author | Chevalier, R | en_US |
dc.contributor.author | Filippenko, AV | en_US |
dc.contributor.author | Fransson, C | en_US |
dc.contributor.author | Panagia, N | en_US |
dc.contributor.author | Phillips, M | en_US |
dc.contributor.author | Schmidt, B | en_US |
dc.contributor.author | Suntzeff, N | en_US |
dc.contributor.author | Wheeler, JC | en_US |
dc.date.accessioned | 2012-11-26T08:49:14Z | - |
dc.date.available | 2012-11-26T08:49:14Z | - |
dc.date.issued | 1998 | en_US |
dc.identifier.citation | Astrophysical Journal Letters, 1998, v. 509 n. 2 PART 2, p. L117-L120 | en_US |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/175105 | - |
dc.description.abstract | We describe and model high-velocity (≈15,000 km s -1) Lyα and Hα emission from the supernova remnant SNR 1987A seen in 1997 September and October with the Space Telescope Imaging Spectrograph. Part of this emission comes from a reverse shock located at ≈75% of the radius of the inner boundary of the inner circumstellar ring and confined within ± 30° of the equatorial plane. Departure from axisymmetry in the Lyα and Hα emission correlates with that seen in nonthermal radio emission and reveals an asymmetry in the circumstellar gas distribution. We also see diffuse high-velocity Lyα emission from supernova debris inside the reverse shock that may be due to excitation by nonthermal particles accelerated by the shock. | en_US |
dc.language | eng | en_US |
dc.publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 | en_US |
dc.relation.ispartof | Astrophysical Journal Letters | en_US |
dc.subject | Circumstellar Matter | en_US |
dc.subject | Shocks | en_US |
dc.subject | Supernova Remnants | en_US |
dc.title | New Hubble Space Telescope observations of high-velocity Lyα and Hα in SNR 1987A | en_US |
dc.type | Article | en_US |
dc.identifier.email | Pun, CSJ: jcspun@hkucc.hku.hk | en_US |
dc.identifier.authority | Pun, CSJ=rp00772 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.scopus | eid_2-s2.0-3743051827 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-3743051827&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 509 | en_US |
dc.identifier.issue | 2 PART 2 | en_US |
dc.identifier.spage | L117 | en_US |
dc.identifier.epage | L120 | en_US |
dc.publisher.place | United Kingdom | en_US |
dc.identifier.scopusauthorid | Michael, E=7004899413 | en_US |
dc.identifier.scopusauthorid | McCray, R=35954431900 | en_US |
dc.identifier.scopusauthorid | Pun, CSJ=7003931846 | en_US |
dc.identifier.scopusauthorid | Borkowski, K=7005527694 | en_US |
dc.identifier.scopusauthorid | Garnavich, P=7006524172 | en_US |
dc.identifier.scopusauthorid | Challis, P=7004555495 | en_US |
dc.identifier.scopusauthorid | Kirshner, RP=35277140000 | en_US |
dc.identifier.scopusauthorid | Chevalier, R=7101871369 | en_US |
dc.identifier.scopusauthorid | Filippenko, AV=34568722000 | en_US |
dc.identifier.scopusauthorid | Fransson, C=7004051800 | en_US |
dc.identifier.scopusauthorid | Panagia, N=35400629400 | en_US |
dc.identifier.scopusauthorid | Phillips, M=7402770160 | en_US |
dc.identifier.scopusauthorid | Schmidt, B=7402828523 | en_US |
dc.identifier.scopusauthorid | Suntzeff, N=7006255654 | en_US |
dc.identifier.scopusauthorid | Wheeler, JC=7403110438 | en_US |
dc.identifier.issnl | 2041-8205 | - |