[작성자:] ilikeafrica
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The Milky Way’s external disc constrained by 2MASS star counts
— This paper focuses on analyzing the external stellar disc of the…
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HNCO abundances in galaxies: Tracing the evolutionary state of starbursts
ENGLER SUMMAK: {Your English summary here}
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Explore San Francisco in United States
## Introduction to San Francisco San Francisco is located on the west…
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Galaxy Evolution in Local Group Analogs. I.
— The paper focuses on studying galaxy evolution within nearby groups dominated…
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Explore Valparaiso in Chile
## Introduction to Valparaiso Valparaíso is located in Chile’s Valparaíso Region and…
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LOW–MASS GALAXY FORMATION IN COSMOLOGICAL AMR SIMULATIONS: THE EFFECTS OF VARYING THE SUB–GRID PHYSICS PARAMETERS
This paper presents numerical simulations aimed at exploring the effects of varying…
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Explore Faro in Portugal
## Introduction to Faro Faro is located in southern Portugal, capital city…
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The magnetic field structure in NGC 253 in presence of a galactic wind
— {Your English summary here}
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Spiral density wave triggering of star formation in SA and SAB galaxies
ENGLLISH SUMMARY: In this paper, Mart´ınez-Garc´ia et al. investigate star formation triggered…
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2D Kinematics and physical properties of 1.0 <∼z <∼1.5 star-forming galaxies⋆
This paper combines two-dimensional kinematic and morphology information on Hα emission obtained…
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A brief guide to FXCOR
This paper discusses FXCOR, a Fourier cross-correlation method developed by Tonry &…
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Explore Mexico City in Mexico
## Introduction to Mexico City Mexico City is located within the Valley…
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Star-forming regions in the intragroup medium of compact groups of galaxies
ENGLISH SSURE: — Title: Multi-wavelength study of compact groups of galaxies: evolutionary…
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Stars quenching stars: how photoionization by local sources regulates gas cooling and galaxy formation
In this letter, Cantalupe argues that the missing ingredient in current models…
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The clustering and evolution of Hα emitters at z ∼1 from HiZELS⋆
The paper investigates the clustering properties of Hα emitters at z =…
