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RISS 인기검색어
- 검색키워드
- 저자 : Eracleous, M. (검색결과 2 건)
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MULTI-SIGHTLINE OBSERVATION OF NARROW ABSORPTION LINES IN LENSED QUASAR SDSS J1029+2623
Misawa, Toru,Saez, Cristian,Charlton, Jane C.,Eracleous, Michael,Chartas, George,Bauer, Franz E.,Inada, Naohisa,Uchiyama, Hisakazu American Astronomical Society 2016 The Astrophysical journal Vol.825 No.1
<P>We exploit the widely separated images of the lensed quasar SDSS J1029+2623 (z(em) = 2.197, theta = 22.'' 5) to observe its outflowing wind through two different sightlines. We present an analysis of three observations, including two with the Subaru telescope in 2010 February and 2014 April, separated by four years, and one with the Very Large Telescope, separated from the second Subaru observation by similar to 2 months. We detect 66 narrow absorption lines (NALs), of which 24 are classified as intrinsic NALs that are physically associated with the quasar based on partial coverage analysis. The velocities of intrinsic NALs appear to cluster around values of v(ej) similar to 59,000, 43,000, and 29,000 km s(-1), which is reminiscent of filamentary structures obtained by numerical simulations. There are no common intrinsic NALs at the same redshift along the two sightlines, implying that the transverse size of the NAL absorbers should be smaller than the sightline distance between two lensed images. In addition to the NALs with large ejection velocities of v(ej) > 1000 km s(-1), we also detect broader proximity absorption lines (PALs) at za(bs) similar to z(em). The PALs are likely to arise in outflowing gas at a distance of r <= 620 pc from the central black hole with an electron density of n(e) >= 8.7 x 10(3) cm(-3). These limits are based on the assumption that the variability of the lines is due to recombination. We discuss the implications of these results on the three-dimensional structure of the outflow.</P>
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Relativistic jet activity from the tidal disruption of a star by a massive black hole
Burrows, D. N.,Kennea, J. A.,Ghisellini, G.,Mangano, V.,Zhang, B.,Page, K. L.,Eracleous, M.,Romano, P.,Sakamoto, T.,Falcone, A. D.,Osborne, J. P.,Campana, S.,Beardmore, A. P.,Breeveld, A. A.,Chester, Nature Publishing Group, a division of Macmillan P 2011 Nature Vol.476 No.7361
Supermassive black holes have powerful gravitational fields with strong gradients that can destroy stars that get too close, producing a bright flare in ultraviolet and X-ray spectral regions from stellar debris that forms an accretion disk around the black hole. The aftermath of this process may have been seen several times over the past two decades in the form of sparsely sampled, slowly fading emission from distant galaxies, but the onset of the stellar disruption event has not hitherto been observed. Here we report observations of a bright X-ray flare from the extragalactic transient Swift J164449.3+573451. This source increased in brightness in the X-ray band by a factor of at least 10,000 since 1990 and by a factor of at least 100 since early 2010. We conclude that we have captured the onset of relativistic jet activity from a supermassive black hole. A companion paper comes to similar conclusions on the basis of radio observations. This event is probably due to the tidal disruption of a star falling into a supermassive black hole, but the detailed behaviour differs from current theoretical models of such events.
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