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相关论文: Spiral Structure Boosts Star Formation in Disk Gal…

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Spiral arms are some of the most spectacular features in disc galaxies, and also present in our own Milky Way. It has been argued that star formation should proceed more efficiently in spiral arms as a result of gas compression. Yet,…

Understanding the effect spiral structure has on star formation properties of galaxies is important to completing our picture of spiral structure evolution. Previous studies have investigated connections between spiral arm properties with…

星系天体物理 · 物理学 2022-08-17 R. Porter-Temple , B. W. Holwerda , A. M. Hopkins , L. E. Porter , C. Henry , T. Geron , B. Simmons , K. Masters , S. Kruk

Spiral-driven instabilities may drive gas inflow to enhance central star formation in disk galaxies. We investigate this hypothesis using the Sloan Digital Sky Survey (SDSS) in a sample of 2779 nearby unbarred star-forming main-sequence…

星系天体物理 · 物理学 2022-05-11 Si-Yue Yu , Dewang Xu , Luis C. Ho , Jing Wang , Wei-Bo Kao

We use hydrodynamic simulations to study the effect of spiral arms on the star formation rate (SFR) occurring in nuclear rings of barred-spiral galaxies. We find that spiral arms can be an efficient means of gas transport from the outskirts…

星系天体物理 · 物理学 2015-06-22 Woo-Young Seo , Woong-Tae Kim

We have examined the ratio between the integrated luminosity of massive young stellar objects detected by the Red MSX Source (RMS) survey and the mass of molecular clouds in the Galactic Ring Survey region, as a function of Galactocentric…

星系天体物理 · 物理学 2015-06-04 T. J. T. Moore , J. S. Urquhart , L. K. Morgan , M. A. Thompson

We use global MHD galaxy simulations to investigate the effects of spiral arms on the evolution of magnetic fields and star formation within a self-regulated interstellar medium (ISM). The same galaxy is simulated twice: once with…

星系天体物理 · 物理学 2025-06-23 Hector Robinson , James Wadsley , J. A. Sellwood , Ralph E. Pudritz

We have imaged a sample of 20 spiral galaxies in H$\alpha$ and in the near-infrared K band (2.2 um), in order to determine the location and strength of star formation in these objects with respect to perturbations in the old stellar…

天体物理学 · 物理学 2009-11-07 Marc S. Seigar , Phil A. James

We test the influence of spiral arms on the star formation activity of disk galaxies by constructing and fitting multi-wavelength SEDs for the two nearby spiral galaxies NGC 628 and NGC 4321, at a spatial scale of 1-1.5kpc scale. Recent…

星系天体物理 · 物理学 2024-07-11 Bingqing Sun , Daniela Calzetti , Andrew J. Battisti

Spiral arms greatly affect gas flows and star formation in disk galaxies. We use local three-dimensional simulations of the vertically-stratified, self-gravitating, differentially-rotating, interstellar medium (ISM) subject to a stellar…

星系天体物理 · 物理学 2020-07-29 Woong-Tae Kim , Chang-Goo Kim , Eve C. Ostriker

For a long time the consensus has been that star formation rates are higher in the interior of spiral arms in galaxies, compared to inter-arm regions. However, recent studies have found that the star formation inside the arms is not more…

宇宙学与河外天体物理 · 物理学 2015-06-03 Esteban Silva-Villa , Soeren Larsen

What role does Galactic structure play in star formation? We have used the Herschel Hi-GAL compact-clump catalogue to examine trends in evolutionary stage over large spatial scales in the inner Galaxy. We examine the relationship between…

星系天体物理 · 物理学 2018-07-11 S. E. Ragan , T. J. T. Moore , D. J. Eden , M. G. Hoare , J. S. Urquhart , D. Elia , S. Molinari

In order to understand the physical mechanisms underlying non-steady stellar spiral arms in disk galaxies, we analyzed the growing and damping phases of their spiral arms using three-dimensional $N$-body simulations. We confirmed that the…

星系天体物理 · 物理学 2015-06-12 Junichi Baba , Takayuki R. Saitoh , Keiichi Wada

We measure the stellar mass-star formation rate relation in star-forming disk galaxies at z<0.085, using Galaxy~Zoo morphologies to examine different populations of spirals as classified by their kiloparsec-scale structure. We examine the…

We have imaged a sample of 20 face-on spiral galaxies in H\alpha and in the near-IR K-band (2.2 microns), in order to determine the location and strength of star formation with respect to perturbations in the old stellar population. We…

天体物理学 · 物理学 2007-05-23 M. S. Seigar , P. A. James

The role of spiral arms in galaxies -- whether they enhance star formation efficiency or primarily act as material gatherers -- remains an open question. Observational studies have yielded ambiguous results, in part due to the choice of…

星系天体物理 · 物理学 2025-10-07 Bingqing Sun , Daniela Calzetti , Andrew J. Battisti

Spiral arms are common features in low-redshift disc galaxies, and are prominent sites of star-formation and dust obscuration. However, spiral structure can take many forms: from galaxies displaying two strong `grand design' arms, to those…

Spiral arms are the most characteristic features of disc galaxies, easily distinguishable due to their association with ongoing star formation. However, the role of spiral structure in the chemical evolution of galaxies is unclear. Here we…

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…

星系天体物理 · 物理学 2015-06-22 Clare Dobbs , Junichi Baba

By combining two surveys covering a large fraction of the molecular material in the Galactic disk we investigate the role the spiral arms play in the star formation process. We have matched clumps identified by ATLASGAL with their parental…

Context. The origin and nature of spiral arms remain unclear. Star forming regions and young stars are generally strongly associated to the spiral structure, but there are few quantitative predictions from simulations about the involvement…

星系天体物理 · 物理学 2026-01-28 J. Ardèvol , M. Semczuk , T. Antoja , V. P. Debattista , M. Bernet , A. Pettitt
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