Hierarchical Structure of Magnetohydrodynamic Turbulence in Position-position-velocity Space
Burkhart, Blakesley ( Astronomy Department, University of Wisconsin, Madison, 475 N. Charter St., WI 53711, USA ); Lazarian, A. ( Astronomy Department, University of Wisconsin, Madison, 475 N. Charter St., WI 53711, USA ); Goodman, Alyssa ( Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS-78, Cambridge, MA 02138, USA ); Rosolowsky, Erik ( University of British Columbia, Okanagan Campus, 3333 University Way, Kelowna BC V1V 1V7, Canada ) show affiliations
The Astrophysical Journal, Volume 770, Issue 2, article id. 141, 16 pp. (2013).
Published in Jun 2013
Magnetohydrodynamic turbulence is able to create hierarchical structures in the interstellar medium (ISM) that are correlated on a wide range of scales via the energy cascade. We use hierarchical tree diagrams known as dendrograms to characterize structures in synthetic position-position-velocity (PPV) emission cubes of isothermal magnetohydrodynamic turbulence. We show that the structures and degree of hierarchy observed in PPV space are related to the presence of self-gravity and the global sonic and Alfvénic Mach numbers. Simulations with higher Alfvénic Mach number, self-gravity and supersonic flows display enhanced hierarchical structure. We observe a strong dependency on the sonic and Alfvénic Mach numbers and self-gravity when we apply the statistical moments (i.e., mean, variance, skewness, kurtosis) to the leaf and node distribution of the dendrogram. Simulations with self-gravity, larger magnetic field and higher sonic Mach number have dendrogram distributions with higher statistical moments. Application of the dendrogram to three-dimensional density cubes, also known as position-position-position (PPP) cubes, reveals that the dominant emission contours in PPP and PPV are related for supersonic gas but not for subsonic. We also explore the effects of smoothing, thermal broadening, and velocity resolution on the dendrograms in order to make our study more applicable to observational data. These results all point to hierarchical tree diagrams as being a promising additional tool for studying ISM turbulence and star forming regions for obtaining information on the degree of self-gravity, the Mach numbers and the complicated relationship between PPV and PPP data.
Free Keywords: Astrophysics - Galaxy Astrophysics; ISM: structure; magnetohydrodynamics: MHD; turbulence
Astronomy: ISM: structure; magnetohydrodynamics: MHD; turbulence
arXiv: Astrophysics - Galaxy Astrophysics