Results 221 to 230 of about 9,672,606 (254)

Biochef: a client-side WebAssembly-based workflow builder for genomic data analysis. [PDF]

BMC Bioinformatics
Rosa J, Andrade J, Silva JM, Oliveira JL.   +3 more
europepmc   +1 more source

From "Laughing Gas" to "Galaxy Gas": An Updated Review on the Neurological, Pathologic, and Psychiatric Sequelae of Nitrous Oxide Abuse. [PDF]

Cureus
Lal Vallath A, Yadav RP, Bass M, Pippari R, Gnugnoli D.   +4 more
europepmc   +1 more source

Fast radio bursts and the radio perspective on multi-messenger gravitational lensing. [PDF]

Philos Trans A Math Phys Eng Sci
Pastor-Marazuela I.
europepmc   +1 more source

Draft genome sequence of Talaromyces trachyspermus, a biocontrol fungus isolated from broomrape. [PDF]

G3 (Bethesda)
Hemmati R, Dolatabadian A, Saeedi S, Batley J.   +3 more
europepmc   +1 more source

Photometric detection at 7.7 μm of a galaxy beyond redshift 14 with JWST/MIRI. [PDF]

Nat Astron
Helton JM, Rieke GH, Alberts S, Wu Z, Eisenstein DJ, Hainline KN, Carniani S, Ji Z, Baker WM, Bhatawdekar R, Bunker AJ, Cargile PA, Charlot S, Chevallard J, D'Eugenio F, Egami E, Johnson BD, Jones GC, Lyu J, Maiolino R, Pérez-González PG, Rieke MJ, Robertson B, Saxena A, Scholtz J, Shivaei I, Sun F, Tacchella S, Whitler L, Williams CC, Willmer CNA, Willott C, Witstok J, Zhu Y.   +33 more
europepmc   +1 more source

The Galaxy in Context: Structural, Kinematic, and Integrated Properties [PDF]

Annual Review of Astronomy and Astrophysics, 2016
Our Galaxy, the Milky Way, is a benchmark for understanding disk galaxies. It is the only galaxy whose formation history can be studied using the full distribution of stars from faint dwarfs to supergiants.
Joss Bland-Hawthorn, Ortwin Gerhard
exaly   +2 more sources

Some of the next articles are maybe not open access.

Related searches:

Environmental effects on galaxy properties

Astrophysics and Space Science, 2003
This is a study concerning the investigation of galaxy formation and evolution in small-scale structures and the influence of the environment on the properties of galaxies. The environment plays a key role in the evolution of galaxies since it governs the type of encounters.
Rauscher, Laura-Ecaterina, Zeilinger, Werner, Focardi, Paolo, Kelm, B, Rampazzo, Roberto   +4 more
openaire   +2 more sources

Dependence of the clustering properties of galaxies on galaxy age

Chinese Journal of Physics, 2016
Abstract From the Main galaxy data of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10), we construct two volume-limited samples with the luminosity −20.5 ≤ M r  ≤−18.5 and −22.5 ≤ M r  ≤−20.5, respectively, and explore the dependence of the clustering properties of galaxies on galaxy age by cluster analysis.
Xin-Fa Deng, Xiao-Ping Qi, Ping Wu, Peng Jiang, Jun Song, Ying-Ping Ding   +5 more
openaire   +1 more source

Clustering properties of galaxies with different galaxy morphologies

Astroparticle Physics, 2008
Abstract From the volume-limited main galaxy sample of the Sloan Digital Sky Survey Data Release 6 (SDSS DR6), we construct an early-type sample and a late-type sample, and perform comparative studies of clustering properties between them. It is found that the distribution of late-type galaxies is more filamentary.
Xin-Fa Deng, Ji-Zhou He, Jiang Peng, Xiao-Xun Tang, Cheng-Hong Luo   +4 more
openaire   +1 more source

The Dependence of Satellite Galaxy Kinematics on Galaxy Properties

Chinese Astronomy and Astrophysics, 2018
Abstract The relations between the kinematics of satellites and the properties of hosts and satellites themselves are investigated in this paper. Our sample of hosts and satellites is selected from the Sloan Digital Sky Survey (SDSS) data by adopting a self-adapted method developed by van den Bosch et al.
Pei Yuan, Wang Hui-yuan
openaire   +1 more source