SIMBAD references

2014MNRAS.439.1948Y - Mon. Not. R. Astron. Soc., 439, 1948-1958 (2014/April-1)

Tidal-induced lopsidedness in Magellanic-type galaxies.

YOZIN C. and BEKKI K.

Abstract (from CDS):

We investigate the tidally induced conversion of barred late-type spirals to Magellanic-type discs with numerical simulations, to establish how the lifetime of lopsidedness (asymmetry) varies with numerical parametrizations. Using a reference model based on observed properties of the Large Magellanic Cloud (LMC), we show that its off-centre bar, one-arm spiral and one-sided star formation can be induced by a brief tidal interaction. We thereafter perform a detailed parameter study, and find that at the dynamical mass of LMC-type discs ( ∼ 1010 M), stellar lopsidedness (as quantified by the m = 1 Fourier mode) and bar off-centredness can vary widely in amplitude, but are generally short-lived ( ∼ Gyr). Tidal interactions induce more persistent lopsidedness in lower mass galaxies (several Gyr), in particular those with large halo-to-disc mass ratios as implied by recent halo occupation models. We suggest that the tidal interactions play a larger role in the observed ubiquity of lopsidedness than the presently favoured gas accretion mechanism for lower mass galaxies. Other characteristics of Magellanic-type galaxies, such as one-sided star formation, are quantified and tend to arise more prominently in discs with later-type spiral structure (more halo-dominated inner disc, weaker bars) following retrograde orbital encounters.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): galaxies: dwarf - galaxies: interactions - Magellanic Clouds

Simbad objects: 12

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2021.03.02-19:31:52

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