Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Cibulková, Helena"'
Autor:
Cibulková, Helena
Title: Distribution functions of asteroid physical properties Author: Helena Cibulková Institute: Astronomical Institute of Charles University Supervisor: Mgr. Josef Ďurech, Ph.D., Astronomical Institute of Charles Univer- sity Abstract: In this th
Externí odkaz:
http://www.nusl.cz/ntk/nusl-370332
Autor:
Cibulková, Helena, Ďurech, Josef, Vokrouhlický, David, Kaasalainen, Mikko, Oszkiewicz, Dagmara A.
Publikováno v:
A&A 596, A57 (2016)
Context: Large all-sky surveys provide us with a lot of photometric data that are sparse in time (typically few measurements per night) and can be potentially used for the determination of shapes and rotational states of asteroids. The method which i
Externí odkaz:
http://arxiv.org/abs/1610.02790
Autor:
Cibulková, Helena
In this work, we constructed a new model for the collisional evolution of the Main Asteroid Belt. Our goals are to test the scaling law from the work of Benz & Asphaug (1999) and ascertain if it can be used for the whole belt. We want to find initial
Externí odkaz:
http://www.nusl.cz/ntk/nusl-324617
In this work, we construct a new model for the collisional evolution of the main asteroid belt. Our goals are to test the scaling law of Benz and Asphaug (1999) and ascertain if it can be used for the whole belt. We want to find initial size-frequenc
Externí odkaz:
http://arxiv.org/abs/1407.6143
We present an abundance analysis of a sample of 33 hydrogen-rich (DA) white dwarfs. We have used archival high-resolution spectra to measure abundances of calcium, magnesium and iron in a set of 30 objects. In addition, we present preliminary calcium
Externí odkaz:
http://arxiv.org/abs/1012.2639
Autor:
Cibulková, Helena
Publikováno v:
Designum; 2019, Issue 2, p4-10, 7p
Autor:
Cibulková, Helena
In this work, we constructed a new model for the collisional evolution of the Main Asteroid Belt. Our goals are to test the scaling law from the work of Benz & Asphaug (1999) and ascertain if it can be used for the whole belt. We want to find initial
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2186::24bf9dae4d3f2d4e72b2e60ab7cc3575
http://www.nusl.cz/ntk/nusl-324617
http://www.nusl.cz/ntk/nusl-324617
Autor:
Cibulková, Helena
In the present work we study changes of the structure of a star that occur during stellar evolution and the dependence of these changes on the initial mass of the star. Internal changes affect also characteristics of the star which are observable fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::6243c38ba371233e28d3f6ba1b1e03fb
http://www.nusl.cz/ntk/nusl-302068
http://www.nusl.cz/ntk/nusl-302068
Publikováno v:
AIP Conference Proceedings; 3/10/2011, Vol. 1331 Issue 1, p238-245, 8p, 1 Chart, 5 Graphs
Autor:
Cibulková, Helena
Publikováno v:
Designum; 2019, Issue 2, p82-82, 1/2p