Local and global environmental effects on galaxies and active galactic nuclei

This project focuses on ultraviolet light effect in low concentrations of fullerenes, in the top layer of sandy soil and in ultrapure water1. Environmental

It might be tempting to ascribe the loss of baryons to the effects of feedback-driven winds, but there are galaxies that have retained more baryons (bottom-left panel) and where

The circularized stellar mass density profiles for the galaxies in our sample, comparing them with similar mass SDSS ETGs and the massive compact galaxies in Szomoru et al..

By comparing the predicted rotation curves with observations of dwarf and low surface brightness galaxies, we show that the pressure from dark matter annihilation may improve

The analysis of this feature led TDT90 to conclude that strong starbursts should be present in the nuclei of type 2 Seyferts because, despite the weakness or dilution observed in

& Battaner (1989) performed VI broad-band surface photometry on a sample of 13 Seyfert galaxies; they consider two classes: ‘bulge galaxies’ and ‘disc galaxies’ and found that

For this study we have selected four nearby galaxies with confirmed circumnuclear star-forming rings and different nuclear type: Seyfert 1 (NGC 7469), Seyfert 2 (NGC 1068), LINER

Conclusion for 25 Satellites in PAndAS Volume In this first exploration of the planes of satellites in our simulation, considering five different models for the satellite