THE ACCRETING BLACK HOLE SWIFT J1753.5-0127 from RADIO to HARD X-RAY

Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/101556

Title:	THE ACCRETING BLACK HOLE SWIFT J1753.5-0127 from RADIO to HARD X-RAY
Authors:	浦田裕次;Kolehmainen, M.;Corbel, Stephane;Coriat, Mickael;Stern, Daniel;Rahoui, Farid;Kalemci, Emrah;James, Miller-Jones;Kanda, Yuka;Moritani, Yuki;Tomsick, John A.;Migliari, Simone;Urata, Yuji;Harrison, Fiona A.;Miller, Jon M.;Gandhi, Poshak;Yamaoka, Kazutaka;Fürst, Felix;Akitaya, Hiroshi;Uemura, M.;Kaaret, Philip;Huang, Kuiyun;Done, Chris
Contributors:	理學院天文研究所
Keywords:	[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph];accretion;accretion disks – black hole physics – stars: individual (Swift J1753.5–0127) – X-rays: general – X-rays: stars;Astrophysics - High Energy Astrophysical Phenomena;FOS: Physical sciences;High Energy Astrophysical Phenomena (astro-ph.HE);QB460-466 Astrophysics
Date:	2015-07-20
Issue Date:	2026-04-21 14:37:43 (UTC+8)
Publisher:	IOP Publishing Ltd.;American Astronomical Society
Abstract:	摘要： (abridged) We report on multi-wavelength measurements of Swift J1753.5-0127 in the hard state at L=2.7e36 erg/s (assuming d=3 kpc) in 2014. The radio emission is optically thick synchrotron, presumably from a compact jet. We take advantage of the low extinction and model the near-IR to UV emission with a multi-temperature disk model. Assuming a BH mass of M_BH=5 Msun and a system inclination of 40 deg, the fits imply an inner radius for the disk of Rin/Rg>212 d_3 (5Msun/M_BH). The outer radius is R_out/R_g=90,000 d_3 (5Msun/M_BH), which corresponds to 6.6e10 d_3 cm, consistent with the expected size of the disk. The 0.5-240 keV spectrum measured by Swift/XRT, Suzaku, and NuSTAR is relatively well characterized by a power-law with a photon index of Gamma=1.722+/-0.003, but a significant improvement is seen when a second continuum component is added. Reflection is a possibility, but no iron line is detected, implying a low iron abundance. We are able to fit the entire SED with a multi-temperature disk component, a Comptonization component, and a broken power-law, representing the emission from the compact jet. The broken power-law cannot significantly contribute to the soft X-ray emission, and this may be related to why Swift J1753.5-0127 is an outlier in the radio/X-ray correlation. The broken power-law might dominate above 20 keV, which would constrain the break frequency to be between 2.4e10 Hz and 3.6e12 Hz. Although the fits to the full SED do not include significant thermal emission in the X-ray band, previous observations have consistently seen such a component, and we find that there is evidence at the 3.1-sigma level for a disk-blackbody component with a temperature of 150(+30)(-20) eV and an inner radius of 5-14 R_g. If this component is real, it might imply the presence of an inner accretion disk in addition to the strongly truncated (R_in>212 R_g) disk. 18 pages, 9 figures, accepted by ApJ 出版者： American Astronomical Society 出版日期： 2015-07-22 出處： The Astrophysical Journal, 2015-07, Vol.808, p.85- 資源來源： Institute of Physics Journals 識別號： EISSN: 1538-4357 識別號： DOI: 10.48550/arxiv.1506.06780 識別號： DOI: 10.1088/0004-637x/808/1/85
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

Files in This Item:

File	Description	Size	Format
index.html		0Kb	HTML	33	View/Open

社群 sharing

Loading...