Publicación
Variable stars in Local Group Galaxies - II. Sculptor dSph
We present the identification of 634 variable stars in the Milky Way dwarf spheroidal (dSph) satellite Sculptor based on archival ground-based optical...
-
-
PublicaciónVariable stars in local group galaxies - IV. RR Lyrae stars in the central regions of the low-density galaxy Crater IIWe present a search and analysis of variable stars in the recently discovered Crater II dwarf galaxy. Based on B, V, I data collected with the Isaac Newton...
-
PublicaciónVariable stars in Local Group galaxies - V. The fast and early evolution of the low-mass Eridanus II dSph galaxyWe present a detailed study of the variable star population of Eridanus II (Eri II), an ultra-faint dwarf galaxy that lies close to the Milky Way virial radius...
-
PublicaciónVariable Stars in Local Group Galaxies. III. And VII, NGC 147, and NGC 185: Insight into the Building Blocks of the M31 HaloWe present the discovery of 1568 RR Lyrae stars in three of the most luminous M31 satellites: And VII (573), NGC 147 (177), and NGC 185 (818). We use their...
-
PublicaciónVariable stars in Local Group galaxies: VII. New insights into the Leo II dSphAims. Pulsating variable stars are invaluable tracers for reconstructing the star formation history and chemical evolution of their host galaxies. In this work...
-
PublicaciónVariable stars in the Cetus dwarf spheroidal galaxy: population gradients and connections with the star formation historyWe investigate the variable star content of the isolated, Local Group, dwarf spheroidal (dSph) galaxy Cetus. Multi-epoch, wide-field images collected with the...
-
PublicaciónVariable Stars in the Field of the Hydra II Ultra-faint Dwarf GalaxyWe report the discovery of one RR Lyrae star in the ultra-faint satellite galaxy Hydra II based on time series photometry in the g, r and i bands obtained with...
-
PublicaciónVariation of Galactic Bar Length with Amplitude and Density as Evidence for Bar Growth over a Hubble TimeKs-band images of 20 barred galaxies show an increase in the peak amplitude of the normalized m=2 Fourier component with the R25-normalized radius at this peak...
-
PublicaciónVariation of the stellar initial mass function in semi-analytical models. III. Testing the cosmic-ray regulated integrated galaxy-wide initial mass functionContext. In our previous work, we derived the CR-IGIMF, which is a new scenario for a variable stellar initial mass function (IMF) that combines numerical...