A multiwavelength study of spiral structure in galaxies. II. Spiral arms in deep optical observations [PDF]
Monthly notices of the Royal Astronomical Society, 2023 In this paper, we look to analyse the spiral features of grand-design, multiarmed, and flocculent spiral galaxies using deep optical imaging from DESI Legacy Imaging Surveys.
A. Mosenkov +9 more
semanticscholar +1 more source
Evidence for small halos in grand design spiral galaxies
The Astrophysical Journal, 1990 Les courbes de rotation de 41 galaxies spirales de differents types sont comparees. Il est montre que les galaxies ayant deux bras longs et symetriques tendent a avoir des courbes de rotation exterieures tombantes alors que les galaxies ayant des bras multiples ou des bras floconneux courts ont plutot des courbes de rotation presques plates ou s ...
Debra Meloy Elmegreen +1 more
openaire +2 more sources
Synthetic HI observations of a simulated spiral galaxy [PDF]
, 2010 Using the Torus radiative transfer code we produce synthetic observations of the 21 cm neutral hydrogen line from an SPH simulation of a spiral galaxy. The SPH representation of the galaxy is mapped onto an AMR grid, and a ray tracing method is used to ...
Acreman +50 more
core +1 more source
J1649+2635: A Grand-Design Spiral with a Large Double-Lobed Radio Source [PDF]
, 2014 We report the discovery of a grand-design spiral galaxy associated with a double-lobed radio source. J1649+2635 (z = 0.0545) is a red spiral galaxy with a prominent bulge that it is associated with a L(1.4GHz) is approximately 10(exp24) W Hz(exp1) double-
M. Mao +12 more
semanticscholar +1 more source
Simulations of Normal Spiral Galaxies [PDF]
, 2003 Results are presented of numerical simulations of normal isolated late type spiral galaxies. Specifically the galaxy NGC 628 is used as a template. The method employs a TREESPH code including stellar particles, gas particles, cooling and heating of the ...
Bottema, Roelof
core +5 more sources
The host of GRB 171205A in 3D. A resolved multiwavelength study of a rare grand-design spiral GRB host [PDF]
Astronomy & AstrophysicsLong GRB hosts at ...
C. Thone +19 more
semanticscholar +1 more source
A high resolution CO map of the inner region of M51 [PDF]
, 1998 M51, the Whirlpool Galaxy, at a distance of ≈ 9,6 Mpc and a systemic velocity of 465 km s^(−1), is the closest “Grand Design” spiral galaxy. Its low inclination (20°) makes it an excellent target for structural studies, e.g.
Aalto, S. +3 more
core +1 more source
Dawes Review 4: Spiral Structures in Disc Galaxies [PDF]
, 2014 The majority of astrophysics involves the study of spiral galaxies, and stars and planets within them, but how spiral arms in galaxies form and evolve is still a fundamental problem. Major progress in this field was made primarily in the 1960s, and early
Baba, Junichi, Dobbs, Clare
core +1 more source
The Carnegie-Irvine Galaxy Survey. VI. Quantifying Spiral Structure [PDF]
Astrophysical Journal, 2018 The Carnegie-Irvine Galaxy Survey provides high-quality broadband optical images of a large sample of nearby galaxies for detailed study of their structure. To probe the physical nature and possible cosmological evolution of spiral arms, a common feature
Sijie Yu, L. Ho, A. Barth, Zhao-Yu Li
semanticscholar +1 more source
Kinematics of the SN Refsdal host revealed by MUSE: a regularly rotating spiral galaxy at z ≃ 1.5 [PDF]
, 2018 We use Multi Unit Spectroscopic Explorer (MUSE) observations of the galaxy cluster MACS J1149.5+2223 to explore the kinematics of the grand-design spiral galaxy (Sp1149) hosting the supernova 'Refsdal'.
E. D. Teodoro +14 more
semanticscholar +1 more source