Minje Beom

Minje Beom
New Mexico State University | NMSU · Department of Astronomy

Master of Science
PhD candidate in the Department of Astronomy of New Mexico State University

About

7
Publications
56
Reads
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18
Citations
Citations since 2016
7 Research Items
18 Citations
201620172018201920202021202202468101214
201620172018201920202021202202468101214
201620172018201920202021202202468101214
201620172018201920202021202202468101214
Introduction
I am Minje Beom, a Ph.D candidate in the Department of Astronomy of New Mexico State University. My current research field is nearby galaxies using MaNGA (Mapping Nearby Galaxies at APO (Aphache Point Observatory)). Using IFU (Integral Field Unit) spectroscopic data, I am studying galaxy formation and evolution. I also use APO 3.5m telescope photometric data and HST photometric data. (ORCID: https://orcid.org/0000-0002-3032-2292 ) (email: minje.beom@gmail.com)
Additional affiliations
September 2015 - May 2017
Yonsei University
Position
  • Instructor
Description
  • Instructor (‘Understanding of space’, 3hrs/week)
September 2014 - June 2017
Yonsei University
Position
  • Researcher
Education
September 2012 - August 2014
Yonsei University
Field of study
  • Astronomy
March 2005 - August 2012
Yonsei University
Field of study
  • Astronomy

Publications

Publications (7)
Article
Counter-rotating components in galaxies are one of the most direct forms of evidence for past gas accretion or merging. We discovered ten edge-on disk gaseous counter-rotators in a sample of 523 edge-on galaxies identified in the final MaNGA (Mapping Nearby Galaxies at APO) IFU sample. The counter-rotators tend to located in small groups. The gaseo...
Preprint
Full-text available
Counter-rotating components in galaxies are one of the most direct forms of evidence for past gas accretion or merging. We discovered ten edge-on disk gaseous counter-rotators in a sample of 523 edge-on galaxies identified in the final MaNGA (Mapping Nearby Galaxies at APO) IFU sample. The counter-rotators tend to located in small groups. The gaseo...
Preprint
We select 456 galaxies with kinematically misaligned gas and stellar components from 9546 parent galaxies in MaNGA, and classify them into 72 star-forming galaxies, 142 green-valley galaxies and 242 quiescent galaxies. Comparing the spatial resolved properties of the misaligned galaxies with control samples closely match in the D$_n$4000 and stella...
Article
We select 456 galaxies with kinematically misaligned gas and stellar components from 9546 parent galaxies in MaNGA, and classify them into 72 star-forming galaxies, 142 green-valley galaxies and 242 quiescent galaxies. Comparing the spatial resolved properties of the misaligned galaxies with control samples closely match in the Dn4000 and stellar v...
Preprint
Using the integral field unit (IFU) data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, we select a sample of 101 galaxies with counter-rotating stellar disks and regularly-rotating ionized gas disk. We classify the 101 galaxies into four types based on the features of their stellar velocity fields. The relative fractions...
Article
Using the integral field unit data from the Mapping Nearby Galaxies at Apache Point Observatory survey, we select a sample of 101 galaxies with counterrotating stellar disks and regularly rotating ionized gas disks. We classify the 101 galaxies into four types based on the features of their stellar velocity fields. The relative fractions and stella...
Article
The individual characteristics of C, N, O, Na, Mg, Al, Si, and Fe on isochrones have been investigated in this study. Stellar models have been constructed for various mixtures in which the content of each element is changed up to the extreme value reported in recent studies, and the changes in isochrone shape have been analyzed for the various mixt...

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