Results 41 to 50 of about 573 (139)
The nucleus of a galaxy orbits around the mass centroid. Orbital motions appear overstable in numerical experiments started with a galaxy's nucleus at rest atop its mass centroid. The amplitude doubles in 6-10 orbital periods. Orbits precess, nutate, and change their amplitudes, but they keep fairly constant periods.
R. H. Miller, B. F. Smith
openaire +1 more source
This present the first mitochondrial genome dataset for 13 Mesenchytraeus species from the Changbai Mountain glacial refugium. Beyond characterizing standard genomic features, we perform comparative analyses of gene order, nucleotide composition, codon usage, and control region structure.
Juanjuan Chen +4 more
wiley +1 more source
Radio Nuclei in Nearby Galaxies [PDF]
This review is an attempt to summarize VLBI continuum observations at cm- and dm-wavelengths of active galactic nuclei at distances ≲ 100 Mpc (Ho = 50 km s−1 Mpc−1). ‘Nearby galaxies’, thus defined, are close enough for achieving the highest possible spatial resolution.
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The nuclei of bulge-less galaxies [PDF]
Als Beitrag zur Vervollst?andigung unseres Wissens ?uber Galaxienzentren wurde die Zentral-Region sehr sp?ater (bulge-loser) Spiralgalaxien untersucht.
openaire +1 more source
Stellar Populations in the Nuclei of Galaxies.
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Galactic outflows and star-formation quenching: a JWST perspective. [PDF]
Davies RL, Belli S.
europepmc +1 more source
Overmassive black holes and little red dots naturally form in simulations. [PDF]
Chon S +4 more
europepmc +1 more source
Unsupervised multimodal deep learning for galaxy morphology taxonomy: integrating ConvNeXtEmbeddings and morphological parameters for scalable survey science. [PDF]
Selim IM +3 more
europepmc +1 more source
Reduced gas accretion onto galaxies due to effects of external giant radio lobes. [PDF]
Qiu Y, Cen R.
europepmc +1 more source

