L
Ling-Jun Wang
Researcher at Chinese Academy of Sciences
Publications - 93
Citations - 1888
Ling-Jun Wang is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Supernova & Magnetar. The author has an hindex of 23, co-authored 88 publications receiving 1561 citations. Previous affiliations of Ling-Jun Wang include Nanjing University & Beijing Normal University.
Papers
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Journal ArticleDOI
Superluminous supernovae powered by magnetars: late-time light curves and hard emission leakage
TL;DR: In this article, the Lense-Thirring effect due to the Sun's angular momentum and the uncertainty of the Sun quadrupole moment are properly taken into account, and they obtain new upper limits on 5 in the solar system when the LENSE-thirring effects are considered.
Journal Article
Signatures of the circumstellar environment in a normal type Ia supernova
Christopher L. Gerardy,Peter Hoeflich,R. A. Fesen,George H Marion,K. Nomoto,R. M. Quimby,B. E. Schaefer,Ling-Jun Wang,John C Wheeler +8 more
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The most luminous supernova asassn-15lh: signature of a newborn rapidly rotating strange quark star
Zi-Gao Dai,Zi-Gao Dai,Shan-Qin Wang,Shan-Qin Wang,J. S. Wang,J. S. Wang,Ling-Jun Wang,Yun-Wei Yu +7 more
TL;DR: In this article, it was shown that the most luminous supernova discovered very recently, ASASSN-15lh, could have been powered by a newborn ultra-strongly magnetized pulsar, which initially rotates near the Kepler limit.
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X-ray illumination of the ejecta of supernova 1987A.
Josefin Larsson,Claes Fransson,Göran Östlin,Per Gröningsson,Anders Jerkstrand,Cecilia Kozma,Jesper Sollerman,P. Challis,Robert P. Kirshner,Roger A. Chevalier,Kevin Heng,Richard McCray,Nicholas B. Suntzeff,Patrice Bouchet,Arlin P. S. Crotts,J. Danziger,Eli Dwek,P. M. Garnavich,Stephen S. Lawrence,Bruno Leibundgut,Peter Lundqvist,Nino Panagia,C. S. J. Pun,Nathan Smith,George Sonneborn,Ling-Jun Wang,John C Wheeler +26 more
TL;DR: Observations that show the transition to this phase in the supernova SN 1987A in the Large Magellanic Cloud show that the flux started to increase, more than doubling by the end of 2009, and it is shown that this increase is the result of heat deposited by X-rays produced as the ejecta interacts with the surrounding material.
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A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
N. Kuznetsova,Kyle Barbary,B.M. Connolly,A. G. Kim,R. Pain,Natalie A. Roe,Greg Aldering,Rahman Amanullah,Kyle Dawson,Masao Doi,Vitaliy Fadeyev,A. S. Fruchter,R. Gibbons,G. Goldhaber,A. Goobar,Alexander Gude,R. A. Knop,M. Kowalski,C. Lidman,Tomoki Morokuma,J. Meyers,Saul Perlmutter,David Rubin,David J. Schlegel,A. L. Spadafora,Vallery Stanishev,M. Strovink,N. Suzuki,Ling-Jun Wang,Naoki Yasuda +29 more
TL;DR: In this paper, a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7 was presented, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST dataset covering the North GOODS field collected in 2004.