Zobrazeno 1 - 10
of 137
pro vyhledávání: '"Callegari, Simone"'
Background: In water-soluble proteins it is energetically favorable to bury hydrophobic residues and to expose polar and charged residues. In contrast to water soluble proteins, transmembrane proteins face three distinct environments; a hydrophobic l
Externí odkaz:
http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-49473
Publikováno v:
In Clinical Microbiology and Infection May 2023 29(5):610-615
Autor:
Aluicio-Sarduy, Eduardo, Callegari, Simone, del Valle, Diana Gisell Figueroa, Desii, Andrea, Kriegel, Ilka, Scotognella, Francesco
A tuning of the light transmission properties of 1D photonic structures employing an external stimulus is very attracting and opens the way to the fabrication of optical switches for colour manipulation in sensing, lighting, and display technology. W
Externí odkaz:
http://arxiv.org/abs/1804.04491
Autor:
Kazantzidis, Stelios, Mayer, Lucio, Callegari, Simone, Dotti, Massimo, Moustakas, Leonidas A.
Publikováno v:
Astrophys.J. 836 (2017) L13
A conclusive model for the formation of dwarf spheroidal (dSph) galaxies still remains elusive. Owing to their proximity to the massive spirals Milky Way (MW) and M31, various environmental processes have been invoked to explain their origin. In this
Externí odkaz:
http://arxiv.org/abs/1703.08381
Publikováno v:
In Journal of Business Research May 2020 112:271-280
Autor:
Bird, Jonathan C., Kazantzidis, Stelios, Weinberg, David H., Guedes, Javiera, Callegari, Simone, Mayer, Lucio, Madau, Piero
We analyze the present-day structure and assembly history of a high resolution hydrodynamic simulation of the formation of a Milky Way (MW)-like disk galaxy, from the "Eris" simulation suite, dissecting it into cohorts of stars formed at different ep
Externí odkaz:
http://arxiv.org/abs/1301.0620
We study the statistics and cosmic evolution of massive black hole seeds formed during major mergers of gas-rich late-type galaxies. Generalizing the results of the hydro-simulations from Mayer et al. 2010, we envision a scenario in which a supermass
Externí odkaz:
http://arxiv.org/abs/1211.3752
Autor:
Khan, Fazeel Mahmood, Berentzen, Ingo, Berczik, Peter, Just, Andreas, Mayer, Lucio, Nitadori, Keigo, Callegari, Simone
We model for the first time the complete orbital evolution of a pair of Supermassive Black Holes (SMBHs) in a 1:10 galaxy merger of two disk dominated gas-rich galaxies, from the stage prior to the formation of the binary up to the onset of gravitati
Externí odkaz:
http://arxiv.org/abs/1203.1623
Autor:
Van Wassenhove, Sandor, Volonteri, Marta, Mayer, Lucio, Dotti, Massimo, Bellovary, Jillian, Callegari, Simone
Publikováno v:
Astrophys.J.748:L7-L11,2012
Supermassive black holes (SMBHs) have been detected in the centers of most nearby massive galaxies. Galaxies today are the products of billions of years of galaxy mergers, but also billions of years of SMBH activity as active galactic nuclei (AGNs) t
Externí odkaz:
http://arxiv.org/abs/1111.0223
Simulations of the formation of late-type spiral galaxies in a cold dark matter LCDM universe have traditionally failed to yield realistic candidates. Here we report a new cosmological N-body/SPH simulation of extreme dynamic range in which a close a
Externí odkaz:
http://arxiv.org/abs/1103.6030