Results 51 to 60 of about 176,382 (265)

ON THE RADIAL EXTENT OF THE DWARF IRREGULAR GALAXY IC10 [PDF]

open access: yesThe Astrophysical Journal, 2010
7 pages, 4 figures, ApJ Letters ...
Michele Cignoni   +18 more
openaire   +4 more sources

Theoretical predictions for dark matter detection in dwarf irregular galaxies with gamma rays [PDF]

open access: yesPhysical Review D, 2017
We investigate dwarf irregular(dIrr) galaxies as a new category of targets for indirect Dark Matter(DM) searches with gamma-rays. In the framework of point-like analysis, dwarf spheroidal(dSph) galaxies are usually considered as one of the best category ...
V. Gammaldi, E. Karukes, P. Salucci
semanticscholar   +1 more source

Delayed Massive-star Mechanical Feedback at Low Metallicity

open access: yesThe Astrophysical Journal, 2023
The classical model of massive-star mechanical feedback is based on effects at solar metallicity ( Z _⊙ ), yet feedback parameters are very different at low metallicity.
Michelle C. Jecmen, M. S. Oey
doaj   +1 more source

The Stellar Content of 10 Dwarf Irregular Galaxies [PDF]

open access: yesThe Astronomical Journal, 1998
We examine the stellar content of 10 dwarf irregular galaxies of which broad-band CCD photometry was published in Hopp & Schulte-Ladbeck (1995). We also present Halpha images for several of these galaxies. The galaxies in the sample are located outside of the Local Group.
Ulrich Hopp, Regina E. Schulte-Ladbeck
openaire   +3 more sources

The Resilience of Habitable Climates Around Circumbinary Stars

open access: yesJournal of Geophysical Research: Planets, Volume 125, Issue 9, September 2020., 2020
Abstract Here we use a 3‐D climate system model to study the habitability of Earth‐like planets orbiting in circumbinary systems. In the most extreme cases, Earth‐like planets in circumbinary systems could experience variations in the incident stellar flux of up to ~50% on ~100‐day timescales.
Eric T. Wolf   +7 more
wiley   +1 more source

LITTLE THINGS in 3D: robust determination of the circular velocity of dwarf irregular galaxies [PDF]

open access: yes, 2016
Dwarf irregular galaxies (dIrrs) are the smallest stellar systems with extended H I discs. The study of the kinematics of such discs is a powerful tool to estimate the total matter distribution at these very small scales.
G. Iorio   +5 more
semanticscholar   +1 more source

A Study of Two Dwarf Irregular Galaxies with AsymmetricalStar Formation Distributions [PDF]

open access: yes, 2018
Two dwarf irregular galaxies, DDO 187 and NGC 3738, exhibit a striking pattern of star formation: intense star formation is taking place in a large region occupying roughly half of the inner part of the optical galaxy. We use data on the H i distribution
D. Hunter   +25 more
semanticscholar   +1 more source

Near-infrared Stellar Populations in the Metal-poor, Dwarf Irregular Galaxies Sextans A and Leo A [PDF]

open access: yesProceedings of the International Astronomical Union, 2017
We present JHKs observations of the metal-poor ([Fe/H] < −1.40) dwarf-irregular galaxies, Leo A and Sextans A, obtained with the WIYN High-resolution Infrared Camera at Kitt Peak. Their near-IR stellar populations are characterized by using a combination
O. Jones   +5 more
semanticscholar   +1 more source

Shaken, but not expelled: Gentle baryonic feedback from nearby starburst dwarf galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2022
Baryonic feedback is expected to play a key role in regulating the star formation of low-mass galaxies by producing galaxy-scale winds associated with mass-loading factors $\beta\!\sim\!1\!-\!50$.
A. Marasco   +14 more
semanticscholar   +1 more source

Catching Tidal Dwarf Galaxies at a Later Evolutionary Stage with ALFALFA

open access: yesThe Astronomical Journal, 2023
We present deep optical imaging and photometry of four objects classified as “Almost-Dark” galaxies in the Arecibo Legacy Fast Arecibo L-band Feed Array (ALFALFA) survey because of their gas-rich nature and extremely faint or missing optical emission in ...
Laurin M. Gray   +13 more
doaj   +1 more source

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