Results 21 to 30 of about 675,630 (383)
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT We use cosmological simulations of isolated Milky Way (MW)-mass galaxies, as well as Local Group (LG) analogues, to define the ‘edge’ – a caustic manifested in a drop in density or radial velocity – of Galactic-sized haloes, both in dark matter and in stars.
Julio F Navarro +7 more
openaire +4 more sources
The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey [PDF]
, 2004 We utilize Sloan Digital Sky Survey imaging and spectroscopy of ~53,000 star-forming galaxies at z ~ 0.1 to study the relation between stellar mass and gas-phase metallicity.
C. Tremonti +11 more
semanticscholar +1 more source
On galaxies and homology [PDF]
Monthly Notices of the Royal Astronomical Society, 2012 15 pages, 9 figures, 3 tables.
Joel R. Primack +7 more
openaire +6 more sources
Acknowledgement to Reviewers of Galaxies in 2016
Galaxies, 2017 The editors of Galaxies would like to express their sincere gratitude to the following reviewers for assessing manuscripts in 2016.[...]
Galaxies Editorial Office
doaj +1 more source
Equipartition Jet Model for the Seyfert 1 Galaxy 3C120 [PDF]
Journal of Astronomy and Space Sciences, 2003 The motion of 3C120 Jet relative to the core is reasonably uniform and the VLBI scale jet connects outwards to a VLA ˜ 100 kpc scale. We measured the jet width variation from the center and found some indication of a power law which indicates the jet ...
Siek Hyung
doaj +1 more source
Acknowledgement to Reviewers of Galaxies in 2017
Galaxies, 2018 Peer review is an essential part in the publication process, ensuring that Galaxies maintains high quality standards for its published papers [...]
Galaxies Editorial Office
doaj +1 more source
Surface Density of Disk Galaxies in MOND
Universe, 2023 In this paper, we extend a paper by Milgrom (2009, MNRAS 398, 1023) dealing with the existence of a quasi-universal surface density for object of all mass and structure, if they are in the Newtonian regime, i.e., that their mean acceleration is larger ...
Antonino Del Popolo, Morgan Le Delliou
doaj +1 more source
The physical properties of star-forming galaxies in the low-redshift universe [PDF]
, 2003 We present a comprehensive study of the physical properties of ∼ 10 5 galaxies with measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical information extracted from the emission lines with continuum properties, we build ...
J. Brinchmann +8 more
semanticscholar +1 more source
Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
Galaxies, 2022 We present the MATLAB code Spirality, a novel method for measuring spiral arm pitch angles by fitting galaxy images to spiral templates of known pitch. Computation time is typically on the order of 2 min per galaxy, assuming 8 GB of working memory.
Deanna Shields +9 more
doaj +1 more source
The AMIGA sample of isolated galaxies. V. Quantification of the isolation [PDF]
, 2007 The AMIGA project aims to build a well defined and statistically significant reference sample of isolated galaxies in order to estimate the environmental effects on the formation and evolution of galaxies.
Abell +36 more
core +3 more sources