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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F09%3A00322209%21RIV09-AV0-67985815
rdf:type
n10:Vysledek skos:Concept
dcterms:description
Nové hodnoty vlastních pohybů Velkého a Malého Magellanova oblaku odvozené Kallivazalil et al. odhalují neočekávaně rychlý prostorový pohyb Magellanova systému. To může znamenat, že se oblaka přibližují k Mléčné dráze poprvé, což znemožňuje interpretaci tvaru a rychlostí HI v Magellanově proudu, mostu a ve vedoucím rameni pomocí modelů použivajících slapové síly. Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement between the available theoretical models of the Magellanic System and the observations of neutral hydrogen (H I) associated with the LMC and the SMC. We investigated this hypothesis for the pure tidal models, as they were the first ones devised to explain the evolution of the Magellanic System, and the tidal stripping is intrinsically involved in every model assuming the gravitational interaction. Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement between the available theoretical models of the Magellanic System and the observations of neutral hydrogen (H I) associated with the LMC and the SMC. We investigated this hypothesis for the pure tidal models, as they were the first ones devised to explain the evolution of the Magellanic System, and the tidal stripping is intrinsically involved in every model assuming the gravitational interaction.
dcterms:title
Pohyb Magellanových oblaků v prostoru: jsou slapové modely vyloučeny? Spatial motion of the Magellanic clouds: tidal models rulled out? Spatial motion of the Magellanic clouds: tidal models rulled out?
skos:prefLabel
Pohyb Magellanových oblaků v prostoru: jsou slapové modely vyloučeny? Spatial motion of the Magellanic clouds: tidal models rulled out? Spatial motion of the Magellanic clouds: tidal models rulled out?
skos:notation
RIV/67985815:_____/09:00322209!RIV09-AV0-67985815
n3:aktivita
n5:P n5:Z
n3:aktivity
P(KJB300030801), P(LC06014), Z(AV0Z10030501)
n3:cisloPeriodika
2
n3:dodaniDat
n16:2009
n3:domaciTvurceVysledku
n9:1532901 n9:6877656
n3:druhVysledku
n11:J
n3:duvernostUdaju
n17:S
n3:entitaPredkladatele
n18:predkladatel
n3:idSjednocenehoVysledku
342743
n3:idVysledku
RIV/67985815:_____/09:00322209
n3:jazykVysledku
n8:eng
n3:klicovaSlova
galaxies evolution; galaxies interaction; kinematics and dynamics; Magellanic Cculds; methods: N-body simulations
n3:klicoveSlovo
n13:kinematics%20and%20dynamics n13:methods%3A%20N-body%20simulations n13:galaxies%20interaction n13:Magellanic%20Cculds n13:galaxies%20evolution
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[40788974B75F]
n3:nazevZdroje
Astrophysical Journal
n3:obor
n7:BN
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
3
n3:projekt
n6:LC06014 n6:KJB300030801
n3:rokUplatneniVysledku
n16:2009
n3:svazekPeriodika
691
n3:tvurceVysledku
Palouš, Jan Theis, Ch. Růžička, Adam
n3:wos
263304300072
n3:zamer
n14:AV0Z10030501
s:issn
0004-637X
s:numberOfPages
9