Paginacija
- Vretenar, Dario, Nikšić, Tamara, Ring, PeterA microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models
- Benić, Sanjin, Blaschke, David, Alvarez-Castillo, David E., Tobias, Fischer, Typel, StefanA new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
- Horvat, Dubravko, Podobnik, Boris, Tadić, DubravkoA non-hedgehog solution for the chiral bag
- Horvat, Dubravko, Podobnik, Boris, Tadić, DubravkoA non-hedgehog solution for the chiral bag
- Rappaport, S., Lehmann, H., Kalomeni, B., Borkovits, T., Latham, D., Bieryla, A., Ngo, H., Mawet, D., Howell, S., Horch, E., Jacobs, T.L., LaCourse, D., Sodor, A., Vanderburg, A., Pavlovski, KrešimirA quintuple star system containing two eclipsing binaries.
- Pašić, SelimA simple and efficient yet accurate calculation of the double-differential Compton cross section within the impulse approximation
- Pašić, Selim, Gamulin, Ozren, Tocilj, ZoranA simple experimental checking of Heisenberg's uncertainty relations
- Graczyk, D., Smolec, R., Pavlovski, Krešimir, Southworth, J., Pietrzynski, G., Maxted, P.F.L., Konorski, P., Gieren, W., Pilecki, B., Taormina, M., Suchomska, K., Karczmarek, P., Gorski, M., Wielgorski, P., Anderson, R.I.A solar twin in the eclipsing binary LL Aquarii
- Garcia, E. V., Stassun, Keivan G., Pavlovski, Krešimir, Hensberge, Herman, Gómez Maqueo Chew, Y., Claret, A.A strict test of stellar evolution models: the absolute dimensions of the massive benchmark eclipsing binary V578 mon
- Žugec, P., Barbagallo, M., Andrzejewski, J., Perkowski, J., Colonna, N., Bosnar, D., Gawlik, A., Sabaté-Gilarte, M., Bacak, M., Mingrone, F., Chiaveri, E.A synchronization method for the multi-channel silicon telescope
- Riechers, Dominik A., Carilli, Christopher L., Capak, Peter L., Scoville, Nicholas Z., Smolčić, Vernesa, Schinnerer, Eva, Yun, Min, Cox, Pierre, Bertoldi, Frank, Karim, Alexander, Yan, LinALMA Imaging of Gas and Dust in a Galaxy Protocluster at Redshift 5.3: [C II] Emission in "Typical" Galaxies and Dusty Starbursts ≈ 1 Billion Years after the Big Bang
- Pavesi, Riccardo, Riechers, Dominik A., Capak, Peter L., Carilli, Christopher L., Sharon, Chelsea E., Stacey, Gordon J., Karim, Alexander, Scoville, Nicholas Z., Smolčić, VernesaALMA Reveals Weak N ii Emission in "Typical" Galaxies and Intense Starbursts at z = 5–6
Paginacija