Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Lorenzo, Tinacci"'
Autor:
Lorenzo Tinacci, Aurèle Germain, Stefano Pantaleone, Cecilia Ceccarelli, Nadia Balucani, Piero Ugliengo
Publikováno v:
The Astrophysical Journal, Vol 951, Iss 1, p 32 (2023)
Water is one of the most important and abundant molecules in star-forming regions. In protoplanetary disks, where planets and comets form, H _2 O is in a gas or solid form, depending on the dust temperature, i.e., the distance from the center and its
Externí odkaz:
https://doaj.org/article/90376320918d4b86aaf75216b716349a
Autor:
Lorenzo Tinacci, Simón Ferrada-Chamorro, Cecilia Ceccarelli, Stefano Pantaleone, Daniela Ascenzi, Andrea Maranzana, Nadia Balucani, Piero Ugliengo
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 266, Iss 2, p 38 (2023)
The gas-phase reaction networks are the backbone of astrochemical models. However, due to their complexity and nonlinear impact on the astrochemical modeling, they can be the first source of error in the simulations if incorrect reactions are present
Externí odkaz:
https://doaj.org/article/e4bc1b86b486498dbfc0c1ca956712fd
Autor:
Lorenzo, Tinacci, Simón, Ferrada-Chamorro, Cecilia, Ceccarelli, Pantaleone, Stefano, Daniela, Ascenzi, Andrea, Maranzana, Balucani, Nadia, Piero, Ugliengo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3982::f9e590f41f361078201d275b697b05b9
https://hdl.handle.net/11391/1544034
https://hdl.handle.net/11391/1544034
Autor:
Lorenzo Tinacci, Auréle Germain, Stefano Pantaleone, Stefano Ferrero, Cecilia Ceccarelli, Piero Ugliengo
The binding energies (BE) of molecules on the interstellar grains are crucial in the chemical evolution of the interstellar medium (ISM). Both temperature programmed desorption (TPD) laboratory experiments and quantum chemistry computations have ofte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d029ccf12a7730ba32859a1b0021cf15
http://arxiv.org/abs/2205.11954
http://arxiv.org/abs/2205.11954
Publikováno v:
ACS earthspace chemistry. 6(5)
Interstellar grains are composed by a rocky core (usually amorphous silicates) covered by an icy mantle, the most abundant molecule being H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::1750fafceacba6cfb370b44f99442453
https://pubmed.ncbi.nlm.nih.gov/35620318
https://pubmed.ncbi.nlm.nih.gov/35620318
Autor:
Stefano Pantaleone, Andrea Maranzana, Piero Ugliengo, Nadia Balucani, Lorenzo Tinacci, Cecilia Ceccarelli
Publikováno v:
The Astrophysical Journal Supplement Series
Positive ions play a fundamental role in the interstellar chemistry, especially in cold environments where chemistry is believed to be mainly ion-driven. However, in contrast with neutral species, most of the cations present in the astrochemical reac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10e873655ebd929ea927e36b429da2ea
http://arxiv.org/abs/2107.11122
http://arxiv.org/abs/2107.11122
Autor:
Yves-Marie Coïc, Alexandre Chenal, Mahmoud Ghomi, Belén Hernández, Lorenzo Tinacci, Régis Cohen, Santiago Sánchez-Cortés
Publikováno v:
The Journal of Physical Chemistry C. 122:13034-13046
Experimental conditions favoring the tryptophan tight binding to the surface of citrate-reduced gold nanoparticles (Cit-AuNPs) were explored. For this, the adsorption of three molecular compounds, free amino acid (Trp), tripeptide NH2-Gly-Trp-Gly-CON
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9e1d348be552bbc36ecb6368ff530f9f
https://doi.org/10.1021/acs.jpcc.8b02261
https://doi.org/10.1021/acs.jpcc.8b02261
Autor:
'Lorenzo Tinacci
Publikováno v:
Stefano Pantaleone
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r3c4b2081b22::02054ae7dee0bf9f4e53e5d1f08e4df1