ASASSN-15oi: a rapidly evolving, luminous tidal disruption event at 216 Mpc

被引:148
作者
Holoien, T. W. -S. [1 ,2 ]
Kochanek, C. S. [1 ,2 ]
Prieto, J. L. [3 ,4 ]
Grupe, D. [5 ]
Chen, Ping [6 ]
Godoy-Rivera, D. [1 ]
Stanek, K. Z. [1 ,2 ]
Shappee, B. J. [7 ]
Dong, Subo [8 ]
Brown, J. S. [1 ]
Basu, U. [1 ,9 ]
Beacom, J. F. [1 ,2 ,10 ]
Bersier, D. [11 ]
Brimacombe, J. [12 ]
Carlson, E. K. [7 ]
Falco, E. [13 ]
Johnston, E. [13 ]
Madore, B. F. [7 ]
Pojmanski, G. [14 ]
Seibert, M. [7 ]
机构
[1] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
[2] Ohio State Univ, CCAPP, 191 W Woodruff Ave, Columbus, OH 43210 USA
[3] Univ Diego Portales, Fac Ingn, Nucleo Astron, Ave Ejercito 441, Santiago, Chile
[4] Millennium Inst Astrophys, Santiago, Chile
[5] Morehead State Univ, Dept Earth & Space Sci, 235 Martindale Dr, Morehead, KY 40351 USA
[6] Peking Univ, Dept Astron, Yi He Yuan Rd 5, Beijing 100871, Peoples R China
[7] Carnegie Observ, 813 Santa Barbara St, Pasadena, CA 91101 USA
[8] Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Rd 5, Beijing 100871, Peoples R China
[9] Grove City High Sch, 4665 Hoover Rd, Grove City, OH 43123 USA
[10] Ohio State Univ, Dept Phys, 191 Woodruff Ave, Columbus, OH 43210 USA
[11] Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England
[12] Coral Towers Observ, Cairns, Qld 4870, Australia
[13] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[14] Warsaw Univ Astron Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
accretion; accretion discs; black hole physics; galaxies: nuclei; ACTIVE GALACTIC NUCLEI; MAIN-SEQUENCE STAR; BLACK-HOLE MASSES; X-RAY OUTBURST; ULTRAVIOLET-BRIGHT; QUIESCENT GALAXY; DISCOVERY; FLARE; MULTIWAVELENGTH; VARIABILITY;
D O I
10.1093/mnras/stw2272
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present ground-based and Swift photometric and spectroscopic observations of the tidal disruption event (TDE) ASASSN-15oi, discovered at the centre of 2MASX J20390918-3045201 (d similar or equal to 216 Mpc) by the All-Sky Automated Survey for SuperNovae. The source peaked at a bolometric luminosity of L similar or equal to 1.3 x 10(44) erg s(-1) and radiated a total energy of E similar or equal to 6.6 x 10(50) erg over the first similar to 3.5 months of observations. The early optical/UV emission of the source can be fit by a blackbody with temperature increasing from T similar to 2 x 10(4) K to T similar to 4 x 10(4) K while the luminosity declines from L similar or equal to 1.3 x 10(44) erg s(-1) to L similar or equal to 2.3 x 10(43) erg s(-1), requiring the photosphere to be shrinking rapidly. The optical/UV luminosity decline during this period is most consistent with an exponential decline, L proportional to e(-(t-t0)/tau), with tau similar or equal to 46.5 d for t(0) similar or equal to 57241.6 (MJD), while a power-law decline of L proportional to (t - t(0))(-alpha) with t(0) similar or equal to 57 212.3 and alpha = 1.62 provides a moderately worse fit. ASASSN-15oi also exhibits roughly constant soft X-ray emission that is significantly weaker than the optical/UV emission. Spectra of the source show broad helium emission lines and strong blue continuum emission in early epochs, although these features fade rapidly and are not present similar to 3 months after discovery. The early spectroscopic features and colour evolution of ASASSN-15oi are consistent with a TDE, but the rapid spectral evolution is unique among optically selected TDEs.
引用
收藏
页码:3813 / 3828
页数:16
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