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Related papers: Supernova Remnant 1987A: The Latest Report from th…

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We present an update on the results of our monitoring observations of the X-ray remnant of supernova (SN) 1987A with the {\it Chandra X-Ray Observatory}. As of 2002 December, we have performed a total of seven observations of SN 1987A. The…

We have been monitoring the supernova remnant (SNR) 1987A with {\it Chandra} observations since 1999. Here we report on the latest change in the soft X-ray light curve of SNR 1987A. For the last $\sim$1.5 yr (since day $\sim$8000), the soft…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Sangwook Park , Svetozar A. Zhekov , David N. Burrows , Judith L. Racusin , Daniel Dewey , Richard McCray

We report an up-turn in the soft X-ray light curve of supernova remnant (SNR) 1987A in late 2003 (~6200 days after the explosion), as observed with the Chandra X-ray Observatory. Since early 2004, the rapid increase of the 0.5-2 keV band…

Astrophysics · Physics 2009-11-13 Sangwook Park , Svetozar A. Zhekov , David N. Burrows , Richard McCray

We report on the morphological and spectral evolution of SNR 1987A from the monitoring observations with the Chandra/ACIS. As of 2005, the X-ray-bright lobes are continuously brightening and expanding all around the ring. The softening of…

We report on the results of our monitoring program of the X-ray remnant of supernova 1987A with the {\it Chandra X-Ray Observatory}. We have performed two new observations during the {\it Chandra} Cycle 3 period, bringing the total to six…

Astrophysics · Physics 2009-11-10 S. Park , D. N. Burrows , S. A. Zhekov , E. Michael , R. McCray , G. Hasinger

We report on the results of our monitoring program of SNR 1987A with the Chandra X-Ray Observatory. The high resolution images and the spectra from the latest Chandra data suggest that the blast wave has reached the dense inner ring in the…

We have been monitoring Supernova (SN) 1987A with {\it Chandra X-Ray Observatory} since 1999. We present a review of previous results from our {\it Chandra} observations, and some preliminary results from new {\it Chandra} data obtained in…

We discuss the X-ray emission observed from Supernova Remnant 1987A with the Chandra X-ray Observatory. We analyze a high resolution spectrum obtained in 1999 October with the high energy transmission grating (HETG). From this spectrum we…

We discuss the results from deep Chandra LETG observations of the supernova remnant 1987A (SNR 1987A). We find that a distribution of shocks, spanning the same range of velocities (from 300 to 1700 km/s) as deduced in the first part of our…

Based on our Chandra imaging-spectroscopic observations, we present the latest evolution of the X-ray remnant of SN 1987A. Recent changes in the electron temperatures and volume emission measures suggest that the blast wave in SN 1987A is…

High Energy Astrophysical Phenomena · Physics 2024-05-06 Aravind P. Ravi , Sangwook Park , Svetozar A. Zhekov , Salvatore Orlando , Marco Miceli , Kari A. Frank , Patrick S. Broos , David N. Burrows

We report the first results from deep X-ray observations of the SNR 1987A with the Chandra LETG. Temperatures inferred from line ratios range from 0.1 - 2 keV and increase with ionization potential. Expansion velocities inferred from X-ray…

Astrophysics · Physics 2010-03-19 S. A. Zhekov , R. McCray , K. J. Borkowski , D. N. Burrows , S. Park

Based on observations with the $Chandra$ X-ray Observatory, we present the latest spectral evolution of the X-ray remnant of SN 1987A (SNR 1987A). We present a high-resolution spectroscopic analysis using our new deep ($\sim$312 ks)…

High Energy Astrophysical Phenomena · Physics 2021-12-09 Aravind P. Ravi , Sangwook Park , Svetozar A. Zhekov , Marco Miceli , Salvatore Orlando , Kari A. Frank , David N. Burrows

We report on the results of our monitoring program of the remnant of SN 1987A with the Advanced CCD Imaging Spectrometer (ACIS) on board the {\it Chandra X-ray Observatory}. Two new observations have been performed in AO2, bringing the…

We present high resolution Chandra observations of the remnant of SN1987A in the Large Magellanic Cloud. The high angular resolution of the Chandra X-ray Observatory (CXO) permits us to resolve the X-ray remnant. We find that the remnant is…

$\sim$18 yr after the supernova explosion, the blast wave of SNR 1987A is entering the main body of the equatorial circumstellar material, which is causing a dramatic brightening of the remnant. We recently reported the observational…

We report observations of the remnant of Supernova 1987A with the High Resolution Camera (HRC) onboard the Chandra X-ray Observatory. A direct image from the HRC resolves the annular structure of the X-ray remnant, confirming the morphology…

High Energy Astrophysical Phenomena · Physics 2014-11-20 C. -Y. Ng , B. M. Gaensler , S. S. Murray , P. O. Slane , S. Park , L. Staveley-Smith , R. N. Manchester , D. N. Burrows

Updated imaging and photometric results from Chandra observations of SN 1987A, covering the last 16 years, are presented. We find that the 0.5-2 keV light curve has remained constant at ~8x10^-12 erg s^-1 cm^-2 since 9500 days, with the 3-8…

High Energy Astrophysical Phenomena · Physics 2016-09-28 Kari A. Frank , Svetozar A. Zhekov , Sangwook Park , Richard McCray , Eli Dwek , David N. Burrows

We present an analysis of the dispersed spectral data from 11 epochs (March 2011 to September 2018) of supernova remnant (SNR) 1987A observations performed with Chandra. These observations were performed with the High Energy Transmission…

High Energy Astrophysical Phenomena · Physics 2021-03-02 Evan Bray , David N. Burrows , Sangwook Park , Aravind P. Ravi

We present an extended analysis of the deep Chandra LETG and HETG observations of the supernova remnant 1987A (SNR 1987A) carried out in 2007. The global fits to the grating spectra show that the temperature of the X-ray emitting plasma in…

We report on the present stage of SN 1987A as observed by the Chandra X-ray Observatory. We reanalyze published Chandra observations and add three more epochs of Chandra data to get a consistent picture of the evolution of the X-ray fluxes…

High Energy Astrophysical Phenomena · Physics 2015-06-12 E. A. Helder , P. S. Broos , D. Dewey , E. Dwek , R. McCray , S. Park , J. L. Racusin , S. A. Zhekov , D. N. Burrows
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