118 citations · 455 across the 10 of their papers we have counts for
10 papers
Formation of the active star forming region LHA 120-N 44 triggered by tidally-driven colliding HI flows
K. Tsuge, H. Sano, K. Tachihara +7
N44 is the second active site of high mass star formation next to R136 in the Large Magellanic Cloud (LMC). We carried out a detailed analysis of HI at 60 arcsec resolution by usin…
The innate origin of radial and vertical gradients in a simulated galaxy disc
Julio F. Navarro, Cameron Yozin, Nic Loewen +6
We examine the origin of radial and vertical gradients in the age/metallicity of the stellar component of a galaxy disc formed in the APOSTLE cosmological hydrody- namical simulati…
Formation of the Young Massive Cluster R136 triggered by Tidally-driven Colliding HI Flows
Yasuo Fukui, Kisetsu Tsuge, Hidetoshi Sano +4
Understanding of massive cluster formation is one of the important issues of astronomy. By analyzing the HI data, we have identified that the two HI velocity components (L- and D-c…
The global warming of group satellite galaxies
C Yozin, K Bekki
Recent studies adopting , a proxy for specific angular momentum, have highlighted how early-type galaxies (ETGs) are composed of two kinematic classes for which distinc…
Local ultra faint dwarves as a product of Galactic processing during a Magellanic group infall
C. Yozin, K. Bekki
The recent discoveries of ultra-faint dwarf (UFD) galaxies in the vicinity of the Magellanic system supports the expectation from cosmological models that such faint objects exist…
The quenching and survival of ultra-diffuse galaxies in the Coma cluster
C. Yozin, K. Bekki
We conduct the first self-consistent numerical simulations of a recently discovered population of 47 large, faint (ultra-diffuse) galaxies, speculated to lie in the Coma cluster. W…
The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
Cameron Yozin, Kenji Bekki
The underlying mechanisms driving the quenching of dwarf-mass satellite galaxies remain poorly constrained, but recent studies suggest they are particularly inefficient for those s…
Evolution of dust and molecular hydrogen in the Magellanic System
Cameron Yozin, Kenji Bekki
We investigate the evolution of the interstellar medium (ISM) in self-consistent, chemodynamical simulations of the Magellanic Clouds (MCs) during their recent (z<0.3) past. An exp…
Tidal-induced lopsidedness in Magellanic-type galaxies
Cameron Yozin, Kenji Bekki
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 (asymme…
The Fornax dwarf galaxy as a remnant of recent dwarf-dwarf merging in the Local Group
C. Yozin, K. Bekki
We present results from the first numerical analysis to support the hypothesis, first proposed in Coleman et al. (2004), that the Fornax dwarf galaxy was formed from the minor merg…