Results 11 to 20 of about 161 (110)

GIANT MOLECULAR CLOUDS AND STAR FORMATION IN THE NON-GRAND DESIGN SPIRAL GALAXY NGC 6946 [PDF]

open access: bronzeThe Astrophysical Journal, 2012
23 pages, 21 figures, 3 tables.
David Rebolledo   +4 more
  +6 more sources

High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18 [PDF]

open access: greenNature, 2012
Accepted for publication in Nature (July 19 2012).
David R. Law   +5 more
openalex   +8 more sources

High-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51 [PDF]

open access: bronzeAstronomy & Astrophysics, 2014
Accepted for publication in Astronomy & Astrophysics, 23 pages, 15 ...
I. De Looze   +22 more
  +11 more sources

A panchromatic spatially resolved analysis of nearby galaxies – II. The main sequence – gas relation at sub-kpc scale in grand-design spirals [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT In this work, we analyse the connection between gas availability and the position of a region with respect to the spatially resolved main-sequence (MS) relation. Following the procedure presented in Enia et al. (2020), for a sample of five face-on, grand design spiral galaxies located on the MS we obtain estimates of stellar ...
L. Morselli   +15 more
openalex   +9 more sources

Spatially resolved properties of the grand-design spiral galaxy UGC 9837: a case for high-redshift 2-D observations [PDF]

open access: bronzeAstronomy & Astrophysics, 2011
12 pages, 9 figures, accepted for publication in A& ...
K. Viironen   +10 more
openalex   +7 more sources

A grand-design spiral galaxy with an ordered magnetic field at redshift 2.6 as resolved with ALMA and gravitational lensing [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society: Letters
ABSTRACT Magnetic fields play an important role in the evolution of galaxies and in shaping the dynamics of their interstellar medium. However, the formation history of magnetic fields from initial seed-fields to well-ordered systems is not clear.
W. de Roo   +5 more
  +5 more sources

Grand Design vs. Multi-Armed Spiral Galaxies: Dependence on Galaxy Structure [PDF]

open access: green
We developed an algorithm to use Galaxy Zoo 3D spiral arm masks produced by citizen scientist volunteers to semi-automatically classify spiral galaxies as either multi-armed or grand design spirals. Our final sample consists of 299 multi-armed and 245 grand design galaxies.
Beverly J. Smith   +3 more
openalex   +3 more sources

Molecules in galaxies. V - CO observations of flocculent and grand-design spirals

open access: bronzeThe Astrophysical Journal, 1987
New carbon monoxide (1-0) observations of 29 spiral galaxies are presented and combined with previously existing data for 74 galaxies in order to study the dependence of the average CO surface brightness on the spiral-arm class. The total sample shows no significant correlation between the CO surface brightness and the presence or absence of grand ...
A. A. Stark   +2 more
openalex   +3 more sources

Flocculent and grand design spiral galaxies in groups - Time scales for the persistence of grand design spiral structures

open access: bronzeThe Astrophysical Journal, 1983
Spiral arm classifications were made for 261 low-inclination galaxies in groups listed by Huchra and Geller. The fractional occurrence of grand design spiral structure in nonbarred galaxies was found to increase from approx.0.1 to approx.0.6 and then level off as the group crossing rate or galaxy collision rate in a group increases.
Bruce G. Elmegreen, D. M. Elmegreen
openalex   +3 more sources

Analyzing the cosmic architecture in the vicinity of Grand-design and Flocculent spiral galaxies with Local Geometric Index

open access: green, 2023
We explore the environment of 351 grand-design and 541 flocculent spiral galaxies recently identified employing convolutional neural networks from the $17^{th}$ data release of Sloan Digital Sky Survey. We introduce a novel estimator called the Local Geometric Index to quantify the morphology of the local environment of these 892 spirals.
Suman Sarkar   +2 more
openalex   +4 more sources

Home - About - Disclaimer - Privacy