Is the Bardeen-Petterson effect responsible for the warping and precession in NGC 4258?

被引:37
作者
Caproni, A.
Abraham, Z.
Livio, M.
Mosquera Cuesta, H. J.
机构
[1] Univ Cruz Sul, CETEC, BR-01506000 Sao Paulo, Brazil
[2] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508900 Sao Paulo, Brazil
[3] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[4] Ctr Brasileiro Pesquisas Fis, ICRA BR, BR-22290180 Rio De Janeiro, Brazil
[5] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy
关键词
accretion; accretion discs; black hole physics; masers; relativity; galaxies : active; galaxies : individual : NGC 4258;
D O I
10.1111/j.1365-2966.2007.11918.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Strong evidence for the presence of a warped Keplerian accretion disc in NGC 4258 (M 106) has been inferred from the kinematics of water masers detected at subparsec scales. Assuming a power-law accretion disc and using constraints on the disc parameters derived from observational data, we have analysed the relativistic Bardeen-Petterson effect driven by a Kerr black hole as the potential physical mechanism responsible for the disc warping. We found that the Bardeen-Petterson radius is comparable to or smaller than the inner radius of the maser disc (independent of the allowed value for the black hole spin parameter). Numerical simulations for a wide range of physical conditions have shown that the evolution of a misaligned disc due to the Bardeen-Petterson torques usually produces an inner flat disc and a warped transition region with a smooth gradient in the tilt and twist angles. Since this structure is similar to that seen in NGC 425 8, we propose that the Bardeen-Petterson effect may be responsible for the disc warping in this galaxy. We estimated the time-scale necessary for the disc inside of the Bardeen-Petterson radius to align with the black hole's equator, as a function of the black hole spin. Our results show that the Bardeen-Petterson effect can align the disc within a few billion years in the case of NGC4258. Finally, we show that if the observed curvature of the outer anomalous arms in the galactic disc of NGC 4258 is associated with the precession of its radio jet/counterjet, then the Bardeen-Petterson effect can provide the required precession period.
引用
收藏
页码:135 / 142
页数:8
相关论文
共 63 条
[1]   SLIM ACCRETION DISKS [J].
ABRAMOWICZ, MA ;
CZERNY, B ;
LASOTA, JP ;
SZUSZKIEWICZ, E .
ASTROPHYSICAL JOURNAL, 1988, 332 (02) :646-658
[2]   Lense-thirring precession of accretion disks around compact objects [J].
Armitage, PJ ;
Natarajan, P .
ASTROPHYSICAL JOURNAL, 1999, 525 (02) :909-914
[3]   ROTATING BLACK HOLES - LOCALLY NONROTATING FRAMES, ENERGY EXTRACTION, AND SCALAR SYNCHROTRON RADIATION [J].
BARDEEN, JM ;
TEUKOLSKY, SA ;
PRESS, WH .
ASTROPHYSICAL JOURNAL, 1972, 178 (02) :347-+
[4]   LENSE-THIRRING EFFECT AND ACCRETION DISKS AROUND KERR BLACK-HOLES [J].
BARDEEN, JM ;
PETTERSON, JA .
ASTROPHYSICAL JOURNAL, 1975, 195 (02) :L65-L67
[5]   DYNAMO-GENERATED TURBULENCE AND LARGE-SCALE MAGNETIC-FIELDS IN A KEPLERIAN SHEAR-FLOW [J].
BRANDENBURG, A ;
NORDLUND, A ;
STEIN, RF ;
TORKELSSON, U .
ASTROPHYSICAL JOURNAL, 1995, 446 (02) :741-754
[6]   VELOCITY FIELD, ROTATION, AND MASS OF NGC 4258 [J].
BURBIDGE, EM ;
PRENDERGAST, KH ;
BURBIDGE, GR .
ASTROPHYSICAL JOURNAL, 1963, 138 (02) :375-&
[7]   Bardeen-Petterson effect and the disk structure of the Seyfert galaxy NGC 1068 [J].
Caproni, A ;
Abraham, Z ;
Cuesta, HJM .
ASTROPHYSICAL JOURNAL, 2006, 638 (01) :120-124
[8]   Observational evidence of spin-induced precession in active galactic nuclei [J].
Caproni, A ;
Cuesta, HJM ;
Abraham, Z .
ASTROPHYSICAL JOURNAL, 2004, 616 (02) :L99-L102
[9]   THE BRAIDED JETS IN THE SPIRAL GALAXY NGC-4258 [J].
CECIL, G ;
WILSON, AS ;
TULLY, RB .
ASTROPHYSICAL JOURNAL, 1992, 390 (02) :365-&
[10]   The active jet in NGC 4258 and its associated shocks [J].
Cecil, G ;
Greenhill, LJ ;
DePree, CG ;
Nagar, N ;
Wilson, AS ;
Dopita, MA ;
Pérez-Fournon, I ;
Argon, AL ;
Moran, JM .
ASTROPHYSICAL JOURNAL, 2000, 536 (02) :675-696