We present a study of the kinematics of the isolated spiral galaxy NGC 864, using Hα Fabry-Perot data obtained with the Galaxy Hα Fabry-Perot System (GHαFaS)...
Hα kinematics of S4G spiral galaxies - II. Data description and non-circular motions
We present a kinematical study of 29 spiral galaxies included in the Spitzer Survey of Stellar Structure in Galaxies, using Hα Fabry-Perot (FP) data obtained...
Hα star formation rates in massive galaxies at z˜ 1
We present a near-infrared spectroscopic study of a stellar mass selected sample of galaxies at z˜ 1 utilizing the Long-slit Intermediate Resolution Infrared...
Identification of a Turnover in the Initial Mass Function of a Young Stellar Cluster Down to 0.5 M<SUB>J</SUB>
A successful theory of star formation should predict the number of objects as a function of their mass produced through star-forming events. Previous studies in...
Imágenes de Hubble y GRANTECAN ayudan a identificar cómo se formaron las primeras galaxias
Una de las preguntas más interesantes que los astrofísicos han tratado de responder desde hace décadas es cómo y cuándo se formaron las primeras galaxias. En...
Impact of metallicity and star formation rate on the time-dependent, galaxy-wide stellar initial mass function
The stellar initial mass function (IMF) is commonly assumed to be an invariant probability density distribution function of initial stellar masses. These...
Impacts of Bar-driven Shear and Shocks on Star Formation
Bars drive gas inflow. As the gas flows inward, shocks and shear occur along the bar dust lanes. Such shocks and shear can affect the star formation (SF) and...
Infrared images and radio continuum of the H II region G 352.2+0.9.
The component G 352.2+0.9 of the H II region/star forming complex NGC 6357 has been studied using near IR images and VLA radio continuum observations at 6 cm.
Infrared studies of H II regions - The Sharpless regions S148, 184, 198, 206 and 269
The results of a combined near-infrared and IRAS mapping study of five H II regions are presented for which fairly complete information at optical and radio...