Results 121 to 130 of about 49,102 (348)
Properties of bars in the local universe
We studied the fraction and properties of bars in a sample of about 3000 galaxies extracted from SDSS-DR5. This represents a volume limited sample with galaxies located between redshift 0.01-20, and inclination i < 60.
Aguerri, J. A. L. +2 more
core
Feeding with tannin‐rich diets altered the fecal microbial composition and increased the relative abundance of tannin‐degrading microbes. We hypothesize that fecal bacteria and fungi may play important roles in helping herbivores adapt to tannin‐rich diets but respond to different tannin concentrations varies.
Di Zhu +5 more
wiley +1 more source
We present a comprehensive investigation into the influence of stellar bars on star formation (SF) in galaxy pairs, using a large sample of low-redshift galaxies (0.02 < z < 0.08) from the DESI Legacy Imaging Surveys Data Release 8. Our analysis examines
Woong-Bae G. Zee, Suk-Jin Yoon
doaj +1 more source
Intergalactic Stellar Distributions in the Interacting M81/M82 Galaxy Group [PDF]
Wei‐Hsin Sun +8 more
openalex +1 more source
Quantifying the FIR interaction enhancement in paired galaxies [PDF]
The Catalog of Isolated Pairs of Galaxies in the Northern Hemisphere, by Karachentsev (1972), was studied and a well-matched comparison sample taken from the Catalog of Isolated Galaxies, by Karachentseva (1973), in order to quantify the enhanced FIR ...
Sulentic, Jack W., Xu, Cong
core +1 more source
Computers and chess masters: The role of AI in transforming elite human performance
Abstract Advances in Artificial Intelligence (AI) have made significant strides in recent years, often supplementing rather than replacing human performance. The extent of their assistance at the highest levels of human performance remains unclear. We analyse over 11.6 million decisions of elite chess players, a domain commonly used as a testbed for AI
Merim Bilalić, Mario Graf, Nemanja Vaci
wiley +1 more source
The molecular gas content throughout the low-z merger sequence
Exploiting IRAM 30 m CO spectroscopy, we find that SDSS post-merger galaxies display gas fractions and depletion times enhanced by 25-50\%, a mildly increased CO excitation, and standard molecular-to-atomic gas ratios, compared to non-interacting ...
Mark T. Sargent +7 more
doaj +1 more source
Probing the physics of interacting galaxies [PDF]
Harriet Cullen +2 more
openalex +1 more source
1ES 1741+196: a BL Lacertae object in a triplet of interacting galaxies? [PDF]
J. Heidt +4 more
openalex +1 more source
The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models [PDF]
Omid Sameie +8 more
openalex +1 more source

