Results 181 to 190 of about 144,375 (218)

Potential impact of the Sagittarius dwarf galaxy on the formation of young O-rich stars. [PDF]

Nat Commun
Sun T, Bi S, Chen X, Chen Y, Lu YL, Liu C, Buck T, Zhang X, Li T, Li Y, Wu Y, Ge Z, Ye L.   +12 more
europepmc   +1 more source

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

Fujimoto S, Ouchi M, Kohno K, Valentino F, Giménez-Arteaga C, Brammer G, Furtak L, Kohandel M, Oguri M, Pallottini A, Richard J, Zitrin A, Bauer F, Boylan-Kolchin M, Dessauges-Zavadsky M, Egami E, Finkelstein S, Ma Z, Smail I, Watson D, Hutchison T, Rigby J, Welch B, Ao Y, Bradley L, Caminha G, Caputi K, Espada D, Endsley R, Fudamoto Y, González-López J, Hatsukade B, Koekemoer A, Kokorev V, Laporte N, Lee M, Magdis G, Ono Y, Rizzo F, Shibuya T, Shimasaku K, Sun F, Toft S, Umehata H, Wang T, Yajima H.   +45 more
europepmc   +1 more source

Extended hot dust emission around the earliest massive quiescent galaxy

Ji Z, Williams C, Rieke G, Lyu J, Alberts S, Sun F, Helton J, Rieke M, Shivaei I, D'Eugenio F, Tacchella S, Robertson B, Zhu Y, Maiolino R, Bunker A, Sun Y, Willmer C.   +16 more
europepmc   +1 more source

The evolution of the cold interstellar medium in galaxies following a starburst★ [PDF]

Monthly Notices of the Royal Astronomical Society, 2015
VW and KR acknowledge support from the European Research Council Starting Grant SEDmorph (P.I. VW).We present the evolution of dust and molecular gas properties in a sample of 11 z ˜ 0.03 starburst to post-starburst (PSB) galaxies selected to span an age
Kate Rowlands, Elisabete da Cunha, Vivienne Wild   +2 more
exaly   +2 more sources

Starburst Galaxies [PDF]

, 1987
The infrared properties of star-forming galaxies, primarily as determined by the Infrared Astronomy Satellite (IRAS), are compared to X-ray, optical, and radio properties.
Daniel Kunth, Daniel Weedman
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Starburst galaxies – An observer’s view

Astrophysics and Space Science, 2004
Starbursts are the most efficient producers of metals in the Universe at low redshifts. They produce enough energy to drive outflows of material from their disks. This makes them important objects to study in order to understand the chemical evolution not only of the interstellar medium (ISM) in the starburst galaxies themselves, but also of the ...
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Red Post-Starburst Galaxies

Astrophysics and Space Science, 1994
Observations of nearby star-forming regions suggest that the initial mass function is deficient in low-mass stars when the ambient star formation rate is high. We investigate the consequences of a truncated initial mass function on the photometric evolution of star burst galaxies using new models of stellar population synthesis. A major prediction with
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Activity in Liner and Starburst Galaxies

Astrophysics and Space Science, 1993
We find, using narrow-band imaging, a direct spatial coincidence between the location of bright [Fe II] 1.64µm line emission and compact steep spectrum radio sources in the nuclear region of the starburst galaxy NGC 253. For a large sample of active galaxies (starburst, LINER and Seyferts) we also find a strong correlation between the integrated ...
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Starburst Galaxies: An Infrared Perspective

2005
The infrared regime is a key range for studies of starburst galaxies. It contains a rich variety of tracers of the gas, dust, and star-formation activity and enables us to probe deep into dust-enshrouded star-forming regions. Selected results based on diagnostics at near and mid-infrared wavelengths are highlighted.
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The Demographics of Starburst Galaxies

AIP Conference Proceedings, 2005
With the advent of an explosion of new data on star formation rates in galaxies from SDSS, 2DF, GALEX, Spitzer, HST, and an armada of new Hα imaging surveys, we are in the midst of a revolution in our understanding of starbursts and their host galaxies.
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