Zobrazeno 1 - 10
of 457
pro vyhledávání: '"Janković, Marija"'
Autor:
Pearce, Tim D., Krivov, Alexander V., Sefilian, Antranik A., Jankovic, Marija R., Löhne, Torsten, Morgner, Tobias, Wyatt, Mark C., Booth, Mark, Marino, Sebastian
Debris discs are our best means to probe the outer regions of planetary systems. Many studies assume that planets lie at the inner edges of debris discs, akin to Neptune and the Kuiper Belt, and use the disc morphologies to constrain those otherwise-
Externí odkaz:
http://arxiv.org/abs/2311.04265
Autor:
Estrada, Beatriz Campos, Owen, James E., Jankovic, Marija R., Wilson, Anna, Helling, Christiane
Catastrophically evaporating rocky planets provide a unique opportunity to study the composition of small planets. The surface composition of these planets can be constrained via modelling their comet-like tails of dust. In this work, we present a ne
Externí odkaz:
http://arxiv.org/abs/2311.02477
Autor:
Sarap, Nataša B., Janković, Marija M., Krneta Nikolić, Jelena D., Vukanac, Ivana S., Rajačić, Milica M.
Publikováno v:
In Nuclear Engineering and Design October 2024 427
Autor:
Janković, Marija, Sarap, Nataša, Janković, Bojan, Krneta Nikolić, Jelena, Rajačić, Milica, Vukanac, Ivana, Jelić, Ivana, Šljivić-Ivanović, Marija
Publikováno v:
In Nuclear Engineering and Design October 2024 427
Autor:
Priou, Sonia, Kempf, Emmanuelle, Flicoteaux, Rémi, Jankovic, Marija, Chatellier, Gilles, Tournigand, Christophe, Daniel, Christel, Lamé, Guillaume
Publikováno v:
In Health Policy and Technology August 2024 13(3)
Autor:
Janković, Bojan, Janković, Marija, Smičiklas, Ivana, Jović, Mihajlo, Vukanac, Ivana, Mraković, Ana, Manić, Nebojša
Publikováno v:
In Thermochimica Acta June 2024 736
Close-in super-Earths are the most abundant exoplanets known. It has been hypothesized that they form in the inner regions of protoplanetary discs, out of the dust that may accumulate at the boundary between the inner region susceptible to the magnet
Externí odkaz:
http://arxiv.org/abs/2108.12332
Short-period super-Earth-sized planets are common. Explaining how they form near their present orbits requires understanding the structure of the inner regions of protoplanetary discs. Previous studies have argued that the hot inner protoplanetary di
Externí odkaz:
http://arxiv.org/abs/2102.12831
Publikováno v:
In Procedia CIRP 2024 122:467-472