GRAVITATIONALLY INDUCED DENSITY WAKE OF A CIRCULARLY ORBITING OBJECT AS AN INTERPRETATIVE FRAMEWORK OF UBIQUITOUS SPIRALS AND ARCS

作者: Hyosun Kim

DOI: 10.1088/0004-637X/739/2/102

关键词: Pitch angleBondi accretionGeometryDensity contrastBow shock (aerodynamics)Mach numberOrbitRadiusWakePhysics

摘要: An orbiting object in a gas-rich environment creates gravitational density wake containing information about the and its orbit. Using linear perturbation theory, we analyze observable properties of due to circularly moving static homogeneous gaseous medium, order derive Bondi accretion radius rB , orbital distance rp Mach number object. Supersonic motion, producing spiral-onion shell structure, exhibits single-armed Archimedes spiral two-centered circular arcs with respect line sight. The pitch angle, arm width, spacing pattern are entirely determined by arm-interarm contrast is proportional decreasing as function power index ?1. background distribution globally changed from initially uniform centrally concentrated. vertical structure manifested center at location. angular extent motion. Diagnostic probes nonlinear wakes such detached bow shock, absence definite inner boundary, presence turbulent low-density eddies, elongated shapes explained extension analysis. enhancement always /rp independent nonlinearity, suggesting that massive objects can substantially modify distribution.

参考文章(53)
B. Fryxell, K. Olson, P. Ricker, F. X. Timmes, M. Zingale, D. Q. Lamb, P. MacNeice, R. Rosner, J. W. Truran, H. Tufo, Flash: An adaptive mesh hydrodynamics code for modeling astrophysical thermonuclear flashes Astrophysical Journal Supplement Series. ,vol. 131, pp. 273- 334 ,(2000) , 10.1086/317361
F. J. Sánchez-Salcedo, A. Brandenburg, Dynamical friction of bodies orbiting in a gaseous sphere Monthly Notices of the Royal Astronomical Society. ,vol. 322, pp. 67- 78 ,(2001) , 10.1046/J.1365-8711.2001.04061.X
Shin-Yi Lin, Motohide Tamura, Nagayoshi Ohashi, Jeremy Lim, Misato Fukagawa, Paul T. P. Ho, Paul T. P. Ho, Shin-Yi Lin, Possible Molecular Spiral Arms in the Protoplanetary Disk of AB Aurigae The Astrophysical Journal. ,vol. 645, pp. 1297- 1304 ,(2006) , 10.1086/504368
Andres Escala, Richard B. Larson, Paolo S. Coppi, Diego Mardones, The role of gas in the merging of massive black holes in galactic nuclei. II. black hole merging in a nuclear gas disk The Astrophysical Journal. ,vol. 630, pp. 152- 166 ,(2005) , 10.1086/431747
N. Soker, Influences of wide binaries on the structures of planetary nebulae Monthly Notices of the Royal Astronomical Society. ,vol. 270, pp. 774- 780 ,(1994) , 10.1093/MNRAS/270.4.774
Charlie Conroy, Jeremiah P. Ostriker, Thermal Balance in the Intracluster Medium: Is AGN Feedback Necessary? The Astrophysical Journal. ,vol. 681, pp. 151- 166 ,(2008) , 10.1086/587861
Eva Villaver, Mario Livio, THE ORBITAL EVOLUTION OF GAS GIANT PLANETS AROUND GIANT STARS The Astrophysical Journal. ,vol. 705, ,(2009) , 10.1088/0004-637X/705/1/L81
Nikos Mastrodemos, Mark Morris, Bipolar Pre-Planetary Nebulae: Hydrodynamics of Dusty Winds in Binary Systems. II. Morphology of the Circumstellar Envelopes The Astrophysical Journal. ,vol. 523, pp. 357- 380 ,(1999) , 10.1086/307717
F. J. Sánchez-Salcedo, Woong-Tae Kim, Hyosun Kim, Dynamical Friction of Double Perturbers in a Gaseous Medium The Astrophysical Journal. ,vol. 679, ,(2008) , 10.1086/589149