Li rich red giant branch stars in the Galactic bulge

•  Detection of molecular clouds with quasars ( Jenkins et al. 2003 ) and indication of the fractal structure with clumpuscules from CO lines in the galactic plane ( Heithausen,

The separation into in-situ and accreted stars indicates that the negative slope partly origi- nates from the in-situ stars, but the steepening of the gradi- ents in the outer

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

parameters of the binary orbit and the masses of the neutron stars can be measured with very high precision by accurate timing measurements.... The Masses of the Neutron Stars in

The Synoptic All-Sky Infrared Survey will reveal the missing sample of faint red dwarf stars in the local solar neighborhood, and the unprecedented sensitivity over such a wide

The paper is organized as follows: in Section 2, we provide the details of the numerical method, the initial and boundary conditions, including a description of the parameters used

Second, the sample of less massive (M  ≤ 1.5 M  ) giant stars with planets covers the same mass range as the MS pro- genitors and subgiant stars where the metal signature has

The high eccentricity of the planet is uncommon among planetary systems orbiting evolved stars and so is the high lithium abundance in a giant starM. The ingestion by the star of