Infrared light from wandering stars

K such that the original and modified M dwarfs are colour-similar, using the same definition of colour-similar to that defined by Paper 1.. 2007, 2010) to these control spectra gave

The spectra of the Near Infrared Background can show ev- idence of a massive Population III era that persisted to late times if this spectra contains a bump from the strong

We see a trend with mass: low–mass stars (M< 3M  ), that experience only TDU, pro- duce carbon, whereas higher mass objects, whose surface chemistry is dominated by HBB,

Finally, we discuss three potential sites for the acceleration of cosmic rays in massive star winds, (i) wind-embedded shocks, (ii) shocks from colliding winds, and (iii) wind

They discuss different channels, the most favourable being the merger of a He white dwarf (He-WD) with a red giant (RG) star. A fast rotating He-core is expected to be formed after

The planned astrometric space mission JASMINE will provide the exact positions, distances, and proper motions of the Galactic bulge stars.. The missing components, the radial ve-

Helium core masses before and at the end of the second dredge-up for different stellar evolution codes (solid line: STERN, dashed line: KEPLER, dotted line: EVOL) as a function of

The bolometric magnitudes for AGB C-rich stars of known variability type, as indicated, plotted as a function of mass loss rates (see Guandalini et al.. Symbols are described below