... bolometric infrared luminosities (L TIR,8−1000 µm ) oflocalgalaxies have been estimated using a sim- ple polynomial presented by P´erault (1987), obtained assuming a simple blackbody ...
... massive galaxies experience one or more phases of nuclear activity ...scenario of close connection between AGNs and their ...mass and galaxy bulge properties (stellar mass, velocity ...
... investigated the X-ray emission from 2568 normal late-type galaxies over the redshift range z = 0 Y ...within the Chandra Deep Fields ...color and abso- lute V-band magnitudes, to ...
... thank the anonymous referee for a helpful report which improved the ...Smith for allow- ing the pre-publication use ofthe H-ATLAS ...from the endowment of ...
... period for lifespan determination Experiments where the IIS pathway was manipulated at different time points in life, both in ...2002) and Drosophila (Giannakou et al., 2007), have shown that in ...
... XLFs for normal /starburst galaxies in GOODS for sources with X-ray counterparts, and fit the XLFs with linear models using ‘‘traditional’’ techniques, as well as Markov- ...
... explanation ofAGN obscuration does not involve the presence ofthe dusty torus, but rather a parsec-scale ...scenario the torus is identified withthe outer region ...
... In the first SUSHIES sample paper, Leloudas et al. (2015c) dis- cussed the spectroscopic properties of 17 H-poor and 8 H-rich SLSN host ...that the host galaxiesof H-poor ...
... thank the anonymous referee for insight that has substantially improved the quality of this ...DJR and DMA acknowledge the support ofthe UK Science and ...
... growth of supermassive black holes and their host galaxies are thought to be linked, but the precise nature of this symbiotic relationship is still poorly ...observations and ...
... to the tidal bridge between two galax- ies. It is known that the interaction between galaxiesand/or galaxy activity phenomena may enhance the rate ofstar ...consequence ...
... when the argument of a variable IMF is considered to explain the [α/Fe]–stellar mass relation, the proposed IMF is treated as a free parameter (Arrigoni et ...varied with exploratory ...
... that the absence of type 1 AGN in these sam- ples of isolated galaxies is ...1.0 AGN among the 175 active galaxies in our sam- ples. The fraction of ...
... pathological history, no language, intellectual or cultural barriers that could affect ...communication. The patient went to emergency service due to a two- week historyof acute abdominal ...
... explore the detailed physics behind these remarkable properties, Marconi et ...time- and metal- dependent convective hydrodynamic models to derive a theoretical calibration forthe period – ...
... reveals the knee for both populations. This fact allows us to compare the level of [ X / Fe ] in stars from each population formed before and after the main contribution ...
... identification of lines for determining the redshifts was done independently from two methods by three ofthe ...authors. The 2D spectrum was visually scanned to search ...
... ent formation processes at different epochs might have shaped the dwarf galaxy evolution (Lisker 2009), the transformation of low-luminositystar forming systems into ...