Results 11 to 20 of about 130 (116)

Analysis of Resonances in Grand Design Spiral Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2001
49 pages, 24 figures, 2 tables.
Vera-Villamizar, Nelson   +3 more
openaire   +2 more sources

Star formation in grand-design, spiral galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2012
Deep, near-infrared JHK-maps were observed for 10 nearby, grand-design, spiral galaxies using HAWK-I/VLT to study the distribution of young stellar clusters in them and thereby determine whether strong spiral perturbations can influence star formation.
Grosbol, P., Dottori, H.
openaire   +2 more sources

Gas and stellar spiral arms and their offsets in the grand-design spiral galaxy M51 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
Theoretical studies on the response of interstellar gas to a gravitational potential disc with a quasi-stationary spiral arm pattern suggest that the gas experiences a sudden compression due to standing shock waves at spiral arms. This mechanism, called a galactic shock wave, predicts that gas spiral arms move from downstream to upstream of stellar ...
Egusa, Fumi   +3 more
openaire   +2 more sources

PHANGS–JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628

open access: yesThe Astrophysical Journal Letters, 2023
We present a high-resolution view of bubbles within the Phantom Galaxy (NGC 628), a nearby (∼10 Mpc), star-forming (∼2 M _⊙ yr ^−1 ), face-on ( i ∼ 9°) grand-design spiral galaxy.
Ashley. T. Barnes   +53 more
doaj   +1 more source

PHANGS–JWST First Results: A Combined HST and JWST Analysis of the Nuclear Star Cluster in NGC 628

open access: yesThe Astrophysical Journal Letters, 2023
We combine archival Hubble Space Telescope and new James Webb Space Telescope imaging data covering the ultraviolet to mid-infrared regime to morphologically analyze the nuclear star cluster (NSC) of NGC 628, a grand-design spiral galaxy.
Nils Hoyer   +30 more
doaj   +1 more source

GRAND DESIGN AND FLOCCULENT SPIRALS IN THESPITZERSURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G) [PDF]

open access: yesThe Astrophysical Journal, 2011
Spiral arm properties of 46 galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G) were measured at 3.6mu, where extinction is small and the old stars dominate. The sample includes flocculent, multiple arm, and grand design types with a wide range of Hubble and bar types.
Elmegreen, Debra Meloy   +28 more
openaire   +5 more sources

Giant molecular clouds in the non-grand design spiral galaxy NGC 6946 [PDF]

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

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

open access: yesThe 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.
B. G. Elmegreen, D. M. Elmegreen
openaire   +1 more source

Evidence for small halos in grand design spiral galaxies

open access: yesThe 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   +1 more source

The sequence of spiral arm classes: Observational signatures of persistent spiral density waves in grand-design galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2019
AbstractWe investigate how the properties of spiral arms relate to other fundamental galaxy properties. To this end, we use previously published measurements of those properties, and our own measurements of arm-interarm luminosity contrasts for a large sample of galaxies, using 3.6μm images from the Spitzer Survey of Stellar Structure in Galaxies ...
Bittner, A.   +6 more
openaire   +3 more sources

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