Giant and supergiant M, S, and C stars are discussed in this survey of research. Basic properties as determined by spectra, chemical composition, photometry, or variability type are discussed. Space motions and space distributions of cool giants are described. Distribution of these stars in our galaxy and those nearby is discussed. Mira variables in particular are surveyed with emphasis on the following topics: (1) phase lag phenomenon; (2) Mira light curves; (3) variations in color indices; (4) determination of multiple periods; (5) correlations between quantities such as period length, light-curve shape, infrared (IR) excess, and visible and IR color diagram; (6) semiregular (SR) variables and different time scales in SR light variations;...
We present a series of papers with the central theme of molecular band spectrum synthesis of cool s...
Ensemble studies of red-giant stars with exquisite asteroseismic (Kepler), spectroscopic (APOGEE), a...
Abstract: Infrared J and K photometry has been obtained of all red giants in the half square degree ...
We investigate the red supergiant (RSG) content of the SMC and LMC using multi-object spectroscopy o...
Context. In recent years, our understanding of red supergiants has been questioned by strong disagre...
Context. In recent years, our understanding of red supergiants has been questioned by strong disagre...
The onset of variability in red giant stars is studied from the data collected by the `Long-Term Pho...
I will be reviewing three methods to identify late-type giants in extragalactic systems, based on th...
We present an investigation of evolved massive stars in the MCs, in particular of the red supergiant...
From the oscillations in red-giant stars measured in time-series data it is possible to derive more ...
There are three important aspects concerning the study of the red giant and in particular of the asy...
From the oscillations in red-giant stars measured in time-series data it is possible to derive more ...
We present the most comprehensive red supergiant (RSG) sample for the Small Magellanic Cloud (SMC) t...
The content of this thesis derives from three projects conducted during my Ph.D, focusing on both th...
As stars age, they go through stages in their life cycles. After the red giant branch, medium mass s...
We present a series of papers with the central theme of molecular band spectrum synthesis of cool s...
Ensemble studies of red-giant stars with exquisite asteroseismic (Kepler), spectroscopic (APOGEE), a...
Abstract: Infrared J and K photometry has been obtained of all red giants in the half square degree ...
We investigate the red supergiant (RSG) content of the SMC and LMC using multi-object spectroscopy o...
Context. In recent years, our understanding of red supergiants has been questioned by strong disagre...
Context. In recent years, our understanding of red supergiants has been questioned by strong disagre...
The onset of variability in red giant stars is studied from the data collected by the `Long-Term Pho...
I will be reviewing three methods to identify late-type giants in extragalactic systems, based on th...
We present an investigation of evolved massive stars in the MCs, in particular of the red supergiant...
From the oscillations in red-giant stars measured in time-series data it is possible to derive more ...
There are three important aspects concerning the study of the red giant and in particular of the asy...
From the oscillations in red-giant stars measured in time-series data it is possible to derive more ...
We present the most comprehensive red supergiant (RSG) sample for the Small Magellanic Cloud (SMC) t...
The content of this thesis derives from three projects conducted during my Ph.D, focusing on both th...
As stars age, they go through stages in their life cycles. After the red giant branch, medium mass s...
We present a series of papers with the central theme of molecular band spectrum synthesis of cool s...
Ensemble studies of red-giant stars with exquisite asteroseismic (Kepler), spectroscopic (APOGEE), a...
Abstract: Infrared J and K photometry has been obtained of all red giants in the half square degree ...