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Matías Gómez

Researcher at Andrés Bello National University

Publications -  81
Citations -  1647

Matías Gómez is an academic researcher from Andrés Bello National University. The author has contributed to research in topics: Globular cluster & Galaxy. The author has an hindex of 21, co-authored 80 publications receiving 1493 citations. Previous affiliations of Matías Gómez include Pontifical Catholic University of Chile & University of Bonn.

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Cepheid Period-Radius and Period-Luminosity Relations and the Distance to the Large Magellanic Cloud

TL;DR: In this article, the authors used the infrared Barnes-Evans surface brightness technique to derive the radii and distances of 34 Galactic Cepheid variables, including 28 Cepheids, to determine the period-radius (PR) relation.
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Cepheid Period-Radius and Period-Luminosity Relations and the Distance to the LMC

TL;DR: In this paper, the authors used the infrared Barnes-Evans surface brightness technique to derive the radii and distances of 34 Galactic Cepheid variables, including 28 Cepheids.
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The ages, metallicities, and alpha element enhancements of globular clusters in the elliptical ngc 5128: a homogeneous spectroscopic study with gemini/gemini multi-object spectrograph

TL;DR: In this paper, the authors present new integrated light spectroscopy of globular clusters (GCs) in NGC 5128, a nearby giant elliptical galaxy less than 4 Mpc away, in order to measure radial velocities and derive ages, metallicities, and alpha-element abundance ratios.
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The Ages, Metallicities and Alpha Element Enhancements of Globular Clusters in the Elliptical NGC 5128: A Homogeneous Spectroscopic Study with Gemini/GMOS

TL;DR: In this paper, the authors present new integrated light spectroscopy of globular clusters (GCs) in NGC 5128 in order to measure radial velocities and derive ages, metallicities, and alpha-element abundance ratios.
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The Kinematics of the Globular Cluster System of NGC 5128 with a New Large Sample of Radial Velocity Measurements

TL;DR: In this paper, the radial velocity measurements for previously known and newly confirmed globular clusters (GCs) in the nearby massive galaxy NGC 5128 are presented, and a new kinematic analysis of the GC system that extends out to 45' in galactocentric radius.