Results 31 to 40 of about 3,892 (249)

Systematically Measuring Ultradiffuse Galaxies (SMUDGes). IV. Ultradiffuse Satellites of Milky Way Analogs

open access: yesThe Astronomical Journal, 2023
To better understand the formation of large, low-surface-brightness galaxies, we measure the correlation function between ultradiffuse galaxy (UDG) candidates and Milky Way analogs (MWAs).
Hina Goto   +4 more
doaj   +1 more source

Nearby Gas‐rich Low Surface Brightness Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2000
We examine the Fisher-Tully cz<1000 km/s galaxy sample to determine whether it is a complete and representative sample of all galaxy types, including low surface brightness populations, as has been recently claimed. We find that the sample is progressively more incomplete for galaxies with (1) smaller physical diameters at a fixed isophote and (2 ...
Schneider, SE, Schombert, JM
openaire   +3 more sources

Searching in H i for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC

open access: yesThe Astronomical Journal, 2023
A search has been made for 21 cm H i line emission in a total of 350 unique galaxies from two samples whose optical properties indicate they may be massive.
K. O’Neil   +6 more
doaj   +1 more source

The properties of a large sample of low surface brightness galaxies from SDSS [PDF]

open access: bronze, 2009
International audienceA large sample of low surface brightness (LSB) disk galaxies is selected from SDSS with B-band central surface brightness mu0(B) from 22 to 24.5 mag arcsec-2.
Y. C. Liang   +8 more
openalex   +3 more sources

Understanding the Chemical Evolution of Blue Edge-on Low Surface Brightness Galaxies

open access: yesThe Astrophysical Journal, 2023
We present a sample of 330 blue edge-on low surface brightness galaxies (ELSBGs). To understand the chemical evolution of ELSBGs, we derived the gas-phase abundance and the [ α /Fe] ratio.
Tian-wen Cao   +6 more
doaj   +1 more source

Fundamental Properties of the Dark and the Luminous Matter from the Low Surface Brightness Discs

open access: yesUniverse, 2021
Dark matter (DM) is one of the biggest mystery in the Universe. In this review, we start reporting the evidences for this elusive component and discussing about the proposed particle candidates and scenarios for such phenomenon.
Paolo Salucci, Chiara di Paolo
doaj   +1 more source

Low-surface-brightness Galaxies are Missing in the Observed Stellar Mass Function

open access: yesThe Astrophysical Journal, 2023
We investigate the impact of the surface-brightness (SB) limit on the galaxy stellar mass functions (GSMFs) using galaxy catalogs generated from the Horizon Run 5 ( HR5 ) simulation.
Juhan Kim   +10 more
doaj   +1 more source

Dwarf Galaxies as Low Surface Brightness Galaxies [PDF]

open access: yesInternational Astronomical Union Colloquium, 1999
AbstractBecause of the weak correlation between surface brightness and luminosity, as galaxy surveys reach to lower surface brightnesses, increasing numbers of dwarf galaxies are found. Thus, studies of dwarf galaxies are relevant to our understanding of the low surface brightness universe. In particular, studies of nearby LSB dwarfs may help to answer
openaire   +1 more source

PEARLS: Low Stellar Density Galaxies in the El Gordo Cluster Observed with JWST

open access: yesThe Astrophysical Journal, 2023
A full understanding of how unusually large ultradiffuse galaxies (UDGs) fit into our conventional theory of galaxy formation remains elusive, despite the large number of objects identified locally.
Timothy Carleton   +25 more
doaj   +1 more source

Kinematics of Giant Low Surface Brightness Galaxies [PDF]

open access: yesInternational Astronomical Union Colloquium, 1999
AbstractHigh sensitivity H I observations now exist for six giant low surface brightness (LSB) disk galaxies including the two prototypes, Malin 1 (Bothun et al. 1987; Impey & Bothun 1989) and F568-6 (also known as Malin 2; Bothun et al. 1990). Their H I surface brightnesses are generally low, but proportionally not as low as their optical surface ...
openaire   +2 more sources

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