Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Bonfini, Paolo"'
Clinical Quality Language (CQL) has emerged as a standard for rule representation in Clinical Decision Support (CDS) and Electronic Clinical Quality Measurement (eCQM) in healthcare. While open-source reference implementations and a few commercial en
Externí odkaz:
http://arxiv.org/abs/2212.06043
Autor:
Maravelias, Grigoris, Bonanos, Alceste Z., Tramper, Frank, de Wit, Stephan, Yang, Ming, Bonfini, Paolo, Zapartas, Emmanuel, Antoniadis, Konstantinos, Christodoulou, Evangelia, Muñoz-Sanchez, Gonzalo
Mass loss is a key property to understand stellar evolution and in particular for low-metallicity environments. Our knowledge has improved dramatically over the last decades both for single and binary evolutionary models. However, episodic mass loss
Externí odkaz:
http://arxiv.org/abs/2209.06303
Autor:
Maravelias, Grigoris, Bonanos, Alceste Z., Tramper, Frank, de Wit, Stephan, Yang, Ming, Bonfini, Paolo
Publikováno v:
A&A 666, A122 (2022)
(abridged) Mass loss is a key parameter in the evolution of massive stars, with discrepancies between theory and observations and with unknown importance of the episodic mass loss. To address this we need increased numbers of classified sources stars
Externí odkaz:
http://arxiv.org/abs/2203.08125
Autor:
Bonfini, Paolo, Zezas, Andreas, Ashby, Matthew L. N., Willner, Steven P., Maragkoudakis, Alexandros, Kouroumpatzakis, Konstantinos, Sell, Paul. H., Kovlakas, Konstantinos
Publikováno v:
MNRAS, 504, 3831-3861 (2021)
We constrain the mass distribution in nearby, star-forming galaxies with the Star Formation Reference Survey (SFRS), a galaxy sample constructed to be representative of all known combinations of star formation rate (SFR), dust temperature, and specif
Externí odkaz:
http://arxiv.org/abs/2107.00973
Autor:
Kouroumpatzakis, Konstantinos, Zezas, Andreas, Maragkoudakis, Alexandros, Willner, Steven P., Bonfini, Paolo, Ashby, Matthew L. N., Sell, Paul H., Jarrett, Thomas H.
We present new H$\alpha$ photometry for the Star-Formation Reference Survey (SFRS), a representative sample of star-forming galaxies in the local Universe. Combining these data with the panchromatic coverage of the SFRS, we provide calibrations of H$
Externí odkaz:
http://arxiv.org/abs/2107.00974
Autor:
Bílek, Michal, Duc, Pierre-Alain, Cuillandre, Jean-Charles, Gwyn, Stephen, Cappellari, Michele, Bekaert, David V., Bonfini, Paolo, Bitsakis, Theodoros, Paudel, Sanjaya, Krajnović, Davor, Durrell, Patrick R., Marleau, Francine
The morphology of galaxies gives essential constraints on the models of galaxy evolution. The morphology of the features in the low-surface-brightness regions of galaxies has not been fully explored yet because of observational difficulties. Here we
Externí odkaz:
http://arxiv.org/abs/2007.13772
Autor:
Kouroumpatzakis, Konstantinos, Zezas, Andreas, Sell, Paul, Kovlakas, Konstantinos, Bonfini, Paolo, Willner, Steven, Ashby, Matthew, Maragkoudakis, Alexandros, Jarrett, Thomas
X-ray luminosity ($L_X$) originating from high-mass X-ray binaries (HMXBs) is tightly correlated with the host galaxy's star-formation rate (SFR). We explore this connection at sub-galactic scales spanning ${\sim}$7 dex in SFR and ${\sim}$8 dex in sp
Externí odkaz:
http://arxiv.org/abs/2004.09873
Akademický článek
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Autor:
Bonfini, Paolo, Graham, Alister W.
Publikováno v:
ApJ, 829, 81B, 2016
Partially-depleted cores are practically ubiquitous in luminous early-type galaxies (M$_{B}\lesssim-$20.5 mag), and typically smaller than 1 kpc. In one popular scenario, supermassive black hole binaries --- established during dry (i.e. gas-poor) gal
Externí odkaz:
http://arxiv.org/abs/1610.00801
Partially depleted cores, as measured by core-Sersic model "break radii", are typically tens to a few hundred parsecs in size. Here we investigate the unusually large (cusp radius of 4.57 kpc) depleted core recently reported for Holm 15A, the brighte
Externí odkaz:
http://arxiv.org/abs/1506.08560