Results 21 to 30 of about 161 (110)

A panchromatic spatially resolved analysis of nearby galaxies – I. Sub-kpc-scale main sequence in grand-design spirals [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT We analyse the spatially resolved relation between stellar mass (M⋆) and star formation rate (SFR) in disc galaxies (i.e. the main sequence, MS). The studied sample includes eight nearby face-on grand-design spirals, e.g. the descendant of high-redshift, rotationally supported star-forming galaxies.
A. Enia   +11 more
openalex   +5 more sources

The detection of spiral arm modulation in the stellar disk of an optically flocculent and an optically grand design galaxy

open access: green, 2000
Two dimensional Fourier spectra of near-infrared images of galaxies provide a powerful diagnostic tool for the detection of spiral arm modulation in stellar disks. Spiral arm modulation may be understood in terms of interference patterns of outgoing and incoming density wave packets or modes.
I. Puerari   +4 more
  +6 more sources

Spiral arm amplitude variations and pattern speeds in the grand design galaxies M51, M81, and M100

open access: bronzeThe Astrophysical Journal, 1989
In the modal theory of galactic spiral structure, the amplitude of a prominent two-arm spiral pattern should oscillate slightly with galactocentric distance because of an interference between the outward and inward propagating waves. In the stellar dynamical theory, the spiral arm amplitudes should oscillate because of differential crowding near and ...
Bruce G. Elmegreen   +2 more
openalex   +3 more sources

A grand-design spiral galaxy 1.5 billion years after the Big Bang with JWST [PDF]

open access: green
11 pages, 2 figures, 2 tables. Comments are welcome.
Rashi Jain, Yogesh Wadadekar
openalex   +3 more sources

Flocculent and grand design spiral arm structure in cluster galaxies [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 1982
D. M. Elmegreen   +2 more
openalex   +3 more sources

THE PdBI ARCSECOND WHIRLPOOL SURVEY (PAWS). I. A CLOUD-SCALE/MULTI-WAVELENGTH VIEW OF THE INTERSTELLAR MEDIUM IN A GRAND-DESIGN SPIRAL GALAXY [PDF]

open access: bronzeThe Astrophysical Journal, 2013
The PdBI (Plateau de Bure Interferometer) Arcsecond Whirlpool Survey (PAWS) has mapped the molecular gas in the central ~9kpc of M51 in its 12CO(1-0) line emission at cloud-scale resolution of ~40pc using both IRAM telescopes. We utilize this dataset to quantitatively characterize the relation of molecular gas (or CO emission) to other tracers of the ...
E. Schinnerer   +12 more
openalex   +7 more sources

PANORAMIC: Discovery of an ultra-massive grand-design spiral galaxy at z∼5.2 [PDF]

open access: closedAstronomy & Astrophysics
We report the discovery of an ultra-massive grand-design red spiral galaxy, named Zhúlóng (Torch Dragon), at zphot = 5.2−0.2+0.3 in the JWST PANORAMIC survey; it is the most distant bulge+disk galaxy candidate with spiral arms known to date. Zhúlóng displays an extraordinary combination of properties: (1) a classical bulge centered in a large, face-on ...
Mengyuan Xiao   +28 more
openalex   +3 more sources

Flocculent and grand design spiral structure in field, binary and group galaxies [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 1982
D. M. Elmegreen, Bruce G. Elmegreen
openalex   +3 more sources

HI and CO spectroscopy of the unusual host of GRB 171205A: A grand design spiral galaxy with a distorted HI field [PDF]

open access: green
GRBs produced by the collapse of massive stars are usually found near the most prominent star-forming regions of star-forming galaxies. GRB 171205A happened in the outskirts of a spiral galaxy, a peculiar location in an atypical GRB host. In this paper we present a highly-resolved study of the molecular gas of this host, with CO(1-0) observations from ...
A. de Ugarte Postigo   +24 more
openalex   +4 more sources

Blue and near-infrared surface photometry of spiral structure in 34 nonbarred grand design and flocculent galaxies

open access: closedThe Astrophysical Journal Supplement Series, 1984
On a examine les profils radiaux du disque et la structure des bras spiraux des 34 galaxies. On donne les profils azimutaux et les diagrammes couleur-amplitude des bras spiraux. On discute des modeles d'evolution de la couleur. Ces modeles sont utilises pour determiner l'amplitude des spirales de densite stellaire sous jacentes et le renforcement ...
D. M. Elmegreen, Bruce G. Elmegreen
openalex   +3 more sources

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