Zobrazeno 1 - 10
of 208
pro vyhledávání: '"Kaňuchová, Z."'
Autor:
Mifsud, D. V., Kaňuchová, Z., Herczku, P., Juhász, Z., Kovács, S. T. S., Lakatos, G., Rahul, K. K., Rácz, R., Sulik, B., Biri, S., Rajta, I., Vajda, I., Ioppolo, S., McCullough, R. W., Mason, N. J.
Publikováno v:
Geophys. Res. Lett., 2022, 49(24), e2022GL100698
The ubiquity of sulfur ions within the Jovian magnetosphere has led to suggestions that the implantation of these ions into the surface of Europa may lead to the formation of SO2. However, previous studies on the implantation of sulfur ions into H2O
Externí odkaz:
http://arxiv.org/abs/2212.08947
Autor:
Migliorini, A., Kanuchova, Z., Ioppolo, S., Barbieri, M., Jones, N. C., Hoffmann, S. V., Strazzulla, G., Tosi, F., Piccioni, G.
Since its first identification on the surface of Ganymede in 1995, molecular oxygen (O2) ice has been at the center of a scientific debate as the surface temperature of the Jovian moon is on average well above the freezing point of O2. Laboratory evi
Externí odkaz:
http://arxiv.org/abs/2205.01659
Autor:
Mifsud, DV, Kaňuchová, Z, Ioppolo, S, Herczku, P, Muiña, A Traspas, Field, TA, Hailey, PA, Juhász, Z, Kovács, STS, Mason, NJ, McCullough, RW, Pavithraa, S, Rahul, KK, Paripás, B, Sulik, B, Chou, SL, Lo, JI, Das, A, Cheng, BM, Rajasekhar, BN, Bhardwaj, A, Sivaraman, B
Publikováno v:
J Mol Spectrosc (2022) 385, 111599
The astrochemistry of CO2 ice analogues has been a topic of intensive investigation due to the prevalence of CO2 throughout the interstellar medium and the Solar System, as well as the possibility of it acting as a carbon feedstock for the synthesis
Externí odkaz:
http://arxiv.org/abs/2203.02847
Autor:
Ioppolo, S., Kanuchová, Z., James, R. L., Dawes, A., Ryabov, A., Dezalay, J., Jones, N. C., Hoffmann, S. V., Mason, N. J., Strazzulla, G.
Publikováno v:
A&A 646, A172 (2021)
Carbonic acid (H2CO3) is a weak acid relevant to astrobiology which, to date, remains undetected in space. Experimental work has shown that the beta-polymorph of H2CO3 forms under space relevant conditions through energetic (UV photon, electron, and
Externí odkaz:
http://arxiv.org/abs/2012.14863
Autor:
Ioppolo, S., Kanuchová, Z., James, R. L., Dawes, A., Jones, N. C., Hoffmann, S. V., Mason, N. J., Strazzulla, G.
Publikováno v:
A&A 641, A154 (2020)
Molecular oxygen, nitrogen, and ozone have been detected in the Solar System. They are also expected to be present in ice-grain mantles within star-forming regions. Laboratory experiments that simulate energetic processing (ions, photons, and electro
Externí odkaz:
http://arxiv.org/abs/2008.01783
Sulfur is an abundant element in the cosmos and it is thus an important contributor to astrochemistry in the interstellar medium and in the Solar System. Astronomical observations of the gas and of the solid phases in the dense interstellar/circumste
Externí odkaz:
http://arxiv.org/abs/1706.08824
Autor:
Woods, Paul M., Occhiogrosso, Angela, Viti, Serena, Kanuchova, Z., Palumbo, Maria Elisabetta, Price, Stephen D.
Sulfur appears to be depleted by an order of magnitude or more from its elemental abundance in star-forming regions. In the last few years, numerous observations and experiments have been performed in order to to understand the reasons behind this de
Externí odkaz:
http://arxiv.org/abs/1503.07227
Autor:
Perna, D., Kaňuchová, Z., Ieva, S., Fornasier, S., Barucci, M. A., Lantz, C., Dotto, E., Strazzulla, G.
Publikováno v:
A&A 575, L1 (2015)
Context: The dwarf planet (1) Ceres - next target of the NASA Dawn mission - is the largest body in the asteroid main belt; although several observations of this body have been performed so far, the presence of surface water ice is still questioned.
Externí odkaz:
http://arxiv.org/abs/1412.5318
Autor:
Mifsud DV; Centre for Astrophysics and Planetary Science, School of Physics and Astronomy, University of Kent, Canterbury CT2 7NH, United Kingdom; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Herczku P; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Ramachandran R; Atomic, Molecular, and Optical Physics Division, Physical Research Laboratory, Ahmedabad 380009, India., Sundararajan P; Atomic, Molecular, and Optical Physics Division, Physical Research Laboratory, Ahmedabad 380009, India., Rahul KK; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Kovács STS; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Sulik B; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Juhász Z; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Rácz R; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Biri S; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary., Kaňuchová Z; Astronomical Institute, Slovak Academy of Sciences, Tatranská Lomnica SK-059 60, Slovakia., Ioppolo S; Centre for Interstellar Catalysis, Department of Physics and Astronomy, Aarhus University, Aarhus DK-8000, Denmark., Sivaraman B; Atomic, Molecular, and Optical Physics Division, Physical Research Laboratory, Ahmedabad 380009, India., McCullough RW; Department of Physics and Astronomy, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, United Kingdom., Mason NJ; Centre for Astrophysics and Planetary Science, School of Physics and Astronomy, University of Kent, Canterbury CT2 7NH, United Kingdom; HUN-REN Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary. Electronic address: n.j.mason@kent.ac.uk.
Publikováno v:
Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy [Spectrochim Acta A Mol Biomol Spectrosc] 2024 Oct 15; Vol. 319, pp. 124567. Date of Electronic Publication: 2024 May 31.
Autor:
Svoren, J., Kanuchova, Z.
Publikováno v:
In Planetary and Space Science 1 October 2018 160:115-119