Orbital structure in barred galaxies

نویسندگان
چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Vertical orbital structure around the Lagrangian points in barred galaxies Link with the secular evolution of galaxies

The stability of the Lagrangian points and the vertical periodic orbits around them is examined in the context of barred galaxies. A transition from stability to complex instability appears for the points L4 and L5 when the strength of the bar is sufficiently large. The Hopf-like bifurcation associated to such a transition is inverse and its effects on the central family of periodic orbits and ...

متن کامل

Barred Galaxies

Theoretical studies suggest that large-scale stellar bars can be highly effective in delivering gas to the central few hundred parsecs of a spiral galaxy, which may then initiate rapid star formation. Further instabilities may lead to additional inflow to physical scales relevant for active galactic nuclei. We test these predictions in light of recent observations. Compared to unbarred spirals,...

متن کامل

Resonances in Barred Galaxies

The inner parts of many spiral galaxies are dominated by bars. These are strong nonaxisymmetric features which significantly affect orbits of stars and dark matter particles. One of the main effects is the dynamical resonances between galactic material and the bar. We detect and characterize these resonances in N-body models of barred galaxies by measuring angular and radial frequencies of indi...

متن کامل

Gas flow in barred galaxies

I briefly review the properties of the gas flow in and around the region of the bar in a disc galaxy and discuss the corresponding inflow and the loci of star formation. I then review the flow of gas in barred galaxies which have an additional secondary bar. Finally I discuss the signatures of bars in edge-on galaxies.

متن کامل

Magnetic fields in barred galaxies

We study the generation and maintenance of large-scale magnetic fields in barred galaxies. We take a velocity field (with strong noncircular components) from a published gas dynamical simulation of Athanassoula (1992), and use this as input to a galactic dynamo calculation. Our work is largely motivated by recent high quality VLA radio observations of the barred galaxy NGC 1097, and we compare ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2007

ISSN: 0035-8711,1365-2966

DOI: 10.1111/j.1365-2966.2007.12263.x