[[abstract]]Elliptical galaxies rotate very slowly, and this rotation affects the way in which gas lost from stars finds its way into the nucleus. It is suggested that the dynamical nature of this flow is the reason why extended double radio sources occur in elliptical galaxies, rather than in spirals. A specific computed example is presented to illustrate the principle, and some observational consequences are discussed. --------------------------------------------------------------------------------[[fileno]]2010118010110[[department]]物理
Recently, we have identified a small number of extended radio sources that consist of two double-lob...
It is commonly accepted that a merger of two spiral galaxies results in a remnant with an elliptica...
Double-double radio galaxies (DDRGs) offer a unique opportunity for us to study multiple episodes of...
For the population of active elliptical galaxies associated with powerful double radio sources, it i...
We present four Mpc-sized radio galaxies which consist of a pair of double-lobed radio sources, alig...
We present four Mpc-sized radio galaxies which consist of a pair of double-lobed radio sources, alig...
The (double) source structure of the radio continuum emission of the more powerful radio sources ass...
We present four Mpc-sized radio galaxies which consist of a pair of double-lobed radio sources, alig...
Aims. We investigate the influence of major mergers on the radio emission of elliptical galaxies. ...
A double-double radio galaxy (DDRG) is defined as consisting of a pair of double radio sources with ...
We describe the pitfalls encountered in deducing from classical double radio source observables (lum...
Double-double radio galaxies (DDRGs) offer a unique opportunity for us to study multiple episodes of...
Using the Illustris simulation, we follow thousands of elliptical galaxies back in time to identify ...
Context. Double-double radio galaxies (DDRGs) represent a short but unique phase in the life-cycle o...
A significant fraction of extended radio sources presents a peculiar X-shaped radio morphology: in a...
Recently, we have identified a small number of extended radio sources that consist of two double-lob...
It is commonly accepted that a merger of two spiral galaxies results in a remnant with an elliptica...
Double-double radio galaxies (DDRGs) offer a unique opportunity for us to study multiple episodes of...
For the population of active elliptical galaxies associated with powerful double radio sources, it i...
We present four Mpc-sized radio galaxies which consist of a pair of double-lobed radio sources, alig...
We present four Mpc-sized radio galaxies which consist of a pair of double-lobed radio sources, alig...
The (double) source structure of the radio continuum emission of the more powerful radio sources ass...
We present four Mpc-sized radio galaxies which consist of a pair of double-lobed radio sources, alig...
Aims. We investigate the influence of major mergers on the radio emission of elliptical galaxies. ...
A double-double radio galaxy (DDRG) is defined as consisting of a pair of double radio sources with ...
We describe the pitfalls encountered in deducing from classical double radio source observables (lum...
Double-double radio galaxies (DDRGs) offer a unique opportunity for us to study multiple episodes of...
Using the Illustris simulation, we follow thousands of elliptical galaxies back in time to identify ...
Context. Double-double radio galaxies (DDRGs) represent a short but unique phase in the life-cycle o...
A significant fraction of extended radio sources presents a peculiar X-shaped radio morphology: in a...
Recently, we have identified a small number of extended radio sources that consist of two double-lob...
It is commonly accepted that a merger of two spiral galaxies results in a remnant with an elliptica...
Double-double radio galaxies (DDRGs) offer a unique opportunity for us to study multiple episodes of...