Search Results - "Blaña, Matías"
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Andromeda chained to the Box – Dynamical Models for M31: Bulge & Bar
Published in Monthly notices of the Royal Astronomical Society (01-05-2017)Get full text
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First Detection of Molecular Gas in the Giant Low Surface Brightness Galaxy Malin 1
Published in Astrophysical journal. Letters (01-11-2024)“…After over three decades of unsuccessful attempts, we report the first detection of molecular gas emission in Malin 1, the largest spiral galaxy observed to…”
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Dwarfs in the Milky Way halo outer rim: first infall or backsplash satellites?
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT Leo T is a gas-rich dwarf located at $414\, {\rm kpc}$ (1.4Rvir) distance from the Milky Way (MW) and it is currently assumed to be on its first…”
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Bar-driven Gas Dynamics of M31
Published in The Astrophysical journal (01-03-2024)“…The large-scale gaseous shocks in the bulge of M31 can be naturally explained by a rotating stellar bar. We use gas dynamical models to provide an independent…”
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Large-scale Hydrodynamical Shocks as the Smoking-gun Evidence for a Bar in M31
Published in The Astrophysical journal (01-07-2022)“…The formation and evolutionary history of M31 are closely related to its dynamical structures, which remain unclear due to its high inclination. Gas kinematics…”
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The Giant Low Surface Brightness Galaxy Malin 1: New Constraints for Its Molecular Gas Mass from GBT/ARGUS Observations
Published in Astrophysical journal. Letters (01-12-2022)“…We report on results from GBT/ARGUS 12 CO(1-0) observations for the giant low surface brightness galaxy Malin 1, which allow us to determine an upper limit for…”
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First Detection of Molecular Gas in the Giant Low Surface Brightness Galaxy Malin 1
Published 01-11-2024“…After over three decades of unsuccessful attempts, we report the first detection of molecular gas emission in Malin 1, the largest spiral galaxy observed to…”
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Unravelling stellar populations in the Andromeda Galaxy
Published 19-01-2021“…A&A 647, A131 (2021) To understand the history and formation mechanisms of galaxies it is crucial to determine their current multidimensional structure. Here…”
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The survey of Planetary Nebulae in Andromeda (M31) II. Age-velocity dispersion relation in the disc from Planetary Nebulae
Published 20-09-2019“…A&A 631, A56 (2019) The age-velocity dispersion relation is an important tool to understand the evolution of the disc of the Andromeda galaxy (M31) in…”
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The Milky Way satellite galaxy Leo T: A perturbed cored dwarf
Published 13-11-2024“…The impact of the dynamical state of gas-rich satellite galaxies at the early moments of their infall into their host systems and the relation to their…”
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A MUSE View of the Core of the Giant Low Surface Brightness Galaxy Malin 1
Published 05-04-2024“…A&A 686, A247 (2024) Aims. The central region of the Giant Low Surface Brightness galaxy Malin 1 has long been known to have a complex morphology with evidence…”
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Dwarfs in the Milky Way halo outer rim: first in-fall or backsplash satellites?
Published 23-07-2020“…Leo T is a gas-rich dwarf located at 414kpc $(1.4R_{\rm vir})$ distance from the Milky Way (MW) and it is currently assumed to be on its first approach. Here,…”
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The giant low surface brightness galaxy Malin 1: new constraints for its molecular gas mass from GBT/ARGUS observations
Published 28-11-2022“…We report on results from GBT/ARGUS $^{12}$CO(1-0) observations for the giant low surface brightness galaxy Malin 1, which allow us to determine an upper limit…”
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Sculpting Andromeda -- made-to-measure models for M31's bar and composite bulge: dynamics, stellar and dark matter mass
Published 22-08-2018“…The Andromeda galaxy (M31) contains a box/peanut bulge (BPB) entangled with a classical bulge (CB) requiring a triaxial modelling to determine the dynamics,…”
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Evidence for non-axisymmetry in M31 from wide-field kinematics of stars and gas
Published 20-07-2017“…A&A 611, A38 (2018) As the nearest large spiral galaxy, M31 provides a unique opportunity to learn about the structure and evolutionary history of this galaxy…”
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Leo IV & V - A possible dwarf galaxy pair ?
Published 05-04-2012“…The last few years have seen the discovery of many faint and ultra-faint dwarf spheroidal galaxies around the Milky Way. Among these is a pair of satellites…”
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Could Segue 1 be a destroyed star cluster? - a dynamical perspective
Published 28-06-2016“…We attempt to find a progenitor for the ultra-faint object Segue 1 under the assumption that it formed as a dark matter free star cluster in the past. We look…”
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Bar-driven Gas Dynamics of M31
Published 08-11-2023“…The large-scale gaseous shocks in the bulge of M31 can be naturally explained by a rotating stellar bar. We use gas dynamical models to provide an independent…”
Get full text
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Large-scale Hydrodynamical Shocks as the Smoking Gun Evidence for a Bar in M31
Published 30-07-2022“…The formation and evolutionary history of M31 are closely related to its dynamical structures, which remain unclear due to its high inclination. Gas kinematics…”
Get full text
Journal Article