Global environmental effects versus galaxy interactions
Texto completo
Figure
Documento similar
The number of H ii regions detected for this galaxy is large enough to explore whether the abundance gradient depends on other properties of the nebular emission.. The H ii
The sign of this slope is in agreement with theoretical expectations (Duffy et al. Concentrations and masses from CLASH. The color of data points and lines encodes the redshift of
Next we study the evolution of the total mass density profiles of the main galaxy clusters in the dataset to find how stable is their mass distribution across their
In this paper, we explore the predicted evolution of basic galaxy morphology.. Median of binned structural parameters Gini, M 20 , and Petrosian radius r P
By studying the distances and angles in spectral space between different galaxy types, it is found that galaxies in the local Universe are distributed along a spectroscopic
Astrometric and photometric star cata- logues derived from the ESA HIPPARCOS Space Astrometry Mission.
The photometry of the 236 238 objects detected in the reference images was grouped into the reference catalog (Table 3) 5 , which contains the object identifier, the right
We here report the properties of Wolf-Rayet (W-R) stars in the nearby spiral galaxy M81. These were found while analysing the slit spectra of a sample of star-forming complexes,