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Your search keyword '"Brož, M."' showing total 334 results

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334 results on '"Brož, M."'

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1. Pebble-driven migration of low-mass planets in the 2D regime of pebble accretion

2. Source regions of carbonaceous meteorites and NEOs

3. Young asteroid families as the primary source of meteorites

4. An advanced multipole model of the (130) Elektra quadruple system

5. Science with a small two-band UV-photometry mission II: Observations of stars and stellar systems

6. 2021 occultations and transits of Linus orbiting (22) Kalliope: I. Polygonal and `cliptracing' algorithm

7. V994 Her: A Unique Triply Eclipsing Sextuple Star System

8. Spectrum of the secondary component and new orbital elements of the massive triple star Delta Ori A

9. The equilibrium shape of (65) Cybele: primordial or relic of a large impact?

10. Towards a consistent model of the hot quadruple system HD 93206 = QZ Carin\ae: II. N-body model

11. Discovery of an asteroid family linked to (22) Kalliope and its moon Linus

12. SPH simulations of high-speed collisions between asteroids and comets

13. Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinae - I. Observations and their initial analyses

14. Observed tidal evolution of Kleopatra's outer satellite

15. Terrestrial planet formation by torque-driven convergent migration of planetary embryos

16. (216) Kleopatra, a low density critically rotating M-type asteroid

17. An advanced multipole model for (216) Kleopatra triple system

18. Optically thin circumstellar medium in $\beta$ Lyr A system

19. Physical and dynamical characterization of the Euphrosyne asteroid Family

20. Binary asteroid (31) Euphrosyne: Ice-rich and nearly spherical

21. Performance of ALICE AD modules in the CERN PS test beam

22. A generator of forward neutrons for ultra-peripheral collisions: $\textbf{n$\mathbf{_O^O}$n}$

23. Impacts into rotating targets: angular momentum draining and efficient formation of synthetic families

24. Properties and nature of Be stars 31. The binary nature, light variability, physical elements, and emission-line changes of HD~81357

25. The shape of (7) Iris as evidence of an ancient large impact?

26. Physical properties of beta Lyr A and its opaque accretion disk

27. SPH/N-body simulations of small (D = 10 km) asteroidal breakups and improved parametric relations for Monte-Carlo collisional models

28. Improved model of the triple system V746 Cas that has a bipolar magnetic field associated with the tertiary

29. An advanced N-body model for interacting multiple stellar systems

30. LHC Forward Physics

33. The origin of long-lived asteroids in the 2:1 mean-motion resonance with Jupiter

34. The thermal emission from boulders on (25143) Itokawa and general implications for the YORP effect

35. Identification and Dynamical Properties of Asteroid Families

37. An anisotropic distribution of spin vectors in asteroid families

38. Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

39. Constraining the cometary flux through the asteroid belt during the late heavy bombardment

40. Investigating the composition of the K[formula omitted] state with π±K[formula omitted] correlations at the LHC

41. Search for the Chiral Magnetic Effect with charge-dependent azimuthal correlations in Xe–Xe collisions at [formula omitted] TeV

42. Inclusive J/psi production in pp collisions at sqrt(s) = 2.76 TeV

43. Did the Hilda collisional family form during the late heavy bombardment?

44. V2368 Oph: An eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Oph

45. A unified solution for the orbit and light-time effect in the V505 Sgr system

47. 2021 occultations and transits of Linus orbiting (22) Kalliope

48. Observation of abnormal suppression of f0(980) production in p–Pb collisions at [formula omitted] = 5.02 TeV

49. Modification of charged-particle jets in event-shape engineered Pb–Pb collisions at [formula omitted] TeV

50. Production of 4He and 4[formula omitted] in Pb–Pb collisions at [formula omitted] at the LHC

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