Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Luboš Neslušan"'
Autor:
Luboš Neslušan, Dušan Tomko
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:3414-3421
There are several groups of comets with perihelion near the solar surface known. Of these, the Marsden and Kracht groups move in orbits situated in a spatial corridor of the daytime Arietid meteoroid stream. The orbits of comets of the Meyer group ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2637ca024e78733a62899790e1c615fb
https://doi.org/10.1093/mnras/stac727
https://doi.org/10.1093/mnras/stac727
Autor:
Tadeusz J. Jopek, Mária Hajduková, Regina Rudawska, Masahiro Koseki, Gulchehra Kokhirova, Luboš Neslušan
Publikováno v:
New Astronomy Reviews. 96:101671
The Shower Database (SD) of the Meteor Data Center (MDC) had been operating on the basis of stream-naming rules which were too complex and insufficiently precise for 15 years. With a gradual increase in the number of discovered meteor showers, the pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5054e0c7f4fc0d4067bf0da47be3c9d
https://doi.org/10.1016/j.newar.2022.101671
https://doi.org/10.1016/j.newar.2022.101671
Autor:
Luboš Neslušan, Mária Hajduková
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 498:1013-1022
We modelled several discrete parts of the meteoroid stream originating in comet C/1853 G1 (Schweizer). In a given model, the orbit of this parent comet was integrated in time backwards for a chosen period (10 000, 20 000, 40 000, or 80 000 yr) and, t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b3117827a9bcfc05913830284fc00f6d
https://doi.org/10.1093/mnras/staa2374
https://doi.org/10.1093/mnras/staa2374
Photometric observations of asteroid (596) Scheila were obtained during and after its 2010 outburst. The estimated radius of the body (spherical approximation of the asteroidal body) was 51.2 km and 50.67 km for different methods. The ejected dust ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9b5a135ca054d978c71d7b4f8cea651
Autor:
Mária Hajduková, Luboš Neslušan
Publikováno v:
Planetary and Space Science. 203:105246
The meteoroid stream of long-period comet C/1861 G1 (Thatcher) is modeled in course to reveal the details of its structure. Specifically, we modeled several parts of the comet's theoretical stream, which were characterized by various values of evolut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2064079a6dfbd9429137799e83cec6f8
https://doi.org/10.1016/j.pss.2021.105246
https://doi.org/10.1016/j.pss.2021.105246
Autor:
Mária Hajduková, Luboš Neslušan
Publikováno v:
The Astronomical Journal. 162:20
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f11c5f712880fe007ef93c6987ccbbdb
https://doi.org/10.3847/1538-3881/abfdc9
https://doi.org/10.3847/1538-3881/abfdc9
Autor:
Luboš Neslušan
Publikováno v:
Planetary and Space Science. 140:1-5
In the past, the formation process of the distant comet Oort Cloud was simulated assuming the ejecting giant planets in their current orbits and with their current masses. Today, it is however known that the planets formed in a tighter configuration
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::88015de13d9b193b8e61becc5d48cedf
https://doi.org/10.1016/j.pss.2017.03.009
https://doi.org/10.1016/j.pss.2017.03.009
Autor:
Mária Hajduková, Luboš Neslušan
Publikováno v:
Planetary and Space Science. 195:105152
We modeled meteoroid streams of two long-period comets, C/1894 G1 (Gale) and C/1936 O1 (Kaho-Kozik-Lis), in order to reveal their possible associations with meteor showers observed in the Earth’s atmosphere. For both comets, we modeled several part
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ada00c3f6df4509cbee62b50936a32dc
https://doi.org/10.1016/j.pss.2020.105152
https://doi.org/10.1016/j.pss.2020.105152
Autor:
M. Hajduková, Luboš Neslušan
Publikováno v:
Icarus. 351:113960
The meteoroid stream of the long-period comet C/1992 W1 (Ohshita) is studied in course to predict and, eventually, confirm the existence of meteor showers originating in this comet. In total, we created 36 models, each representing a part of a theore
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::49d1e70f18ba6f7a043997718c4deaf3
https://doi.org/10.1016/j.icarus.2020.113960
https://doi.org/10.1016/j.icarus.2020.113960