Stellar proper motions in the Galactic bulge from deep Hubble Space Telescope ACS WFC photometry

 The expansionary monetary policy measures have had a negative impact on net interest margins both via the reduction in interest rates and –less powerfully- the flattening of the

Jointly estimate this entry game with several outcome equations (fees/rates, credit limits) for bank accounts, credit cards and lines of credit. Use simulation methods to

The following figures show the evolution along more than half a solar cycle of the AR faculae and network contrast dependence on both µ and the measured magnetic signal, B/µ,

Recent observations of the bulge display a gradient of the mean metallicity and of [Ƚ/Fe] with distance from galactic plane.. Bulge regions away from the plane are less

We present new z- and H-band photometry and proper motion measurements for the five candidate very-low-mass T-type objects we recently proposed to be members of the nearest

In each panel, we show two MDFs derived from the simulations: one based upon the use of all star particles belonging to the bulge, after ap- plication of the kinematic

& Battaner (1989) performed VI broad-band surface photometry on a sample of 13 Seyfert galaxies; they consider two classes: ‘bulge galaxies’ and ‘disc galaxies’ and found that

An example of projected stellar mass density for the disk, spheroid, and galaxy stellar particles is given in Figure 2 for G-1536, as well as the position of the radial cut we use