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star-forming galaxies

The cosmic evolution of star-forming galaxies

The cosmic evolution of star-forming galaxies

... host star-forming galaxies ( Tacchella et ...extinction, star formation rate (SFR) density, and possibly molecular gas ...of galaxies from z < 5, and as such, we will discuss the ...

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Dusty star forming galaxies at high redshift

Dusty star forming galaxies at high redshift

... by star formation, then the sum of our two measured > 3σ 850µm source fluxes, if located at z = 1, would require reradiation of a rest frame ultraviolet sky bright- ness of S ν = 9 × 10 − 25 ergs cm − 2 s − 1 Hz − ...

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Diagnostics for mechanical heating in star-forming galaxies

Diagnostics for mechanical heating in star-forming galaxies

... of star-forming galaxies usually require more than one PDR com- ponent to fit all the ...model star-forming galaxy simulation by assuming the gas density is a log-normal function, in ...

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Chemical evolution of star-forming galaxies in the overdense environment

Chemical evolution of star-forming galaxies in the overdense environment

... in star formation as the galaxy consumes its existing cold gas reser- voir (strangulation, Larson et ...of star formation. Assuming the infall time-scale for galaxies in inner region of the cluster ...

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C III] Emission in Star-Forming Galaxies Near and Far

C III] Emission in Star-Forming Galaxies Near and Far

... MagE galaxies reported here do ...cause galaxies to be strong C III] emitters? For local galaxies, we see that metallicity may set an envelope on maximum C III] equivalent ...metallicity ...

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HR-COSMOS: Kinematics of star-forming galaxies at z ~ 0.9

HR-COSMOS: Kinematics of star-forming galaxies at z ~ 0.9

... of star-forming galaxies in the COSMOS field at intermediate ...(766 galaxies) of morphologically blind galaxies at 0 < z < ...the galaxies in the highest redshift range, ...

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The properties of discrete X-ray sources in star-forming galaxies

The properties of discrete X-ray sources in star-forming galaxies

... candidate star clusters close to/coincident with the X-ray sources within the galaxies, and con- strain the ages of these ...of star clusters to be hindered by high levels of extinction typically ...

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The evolution of star-forming galaxies : analysis of infrared observations by AKARI

The evolution of star-forming galaxies : analysis of infrared observations by AKARI

... the star formation rate at z ∼ ...serving star-forming ...from star formation), with only 10% - 20% contributed by Active Galactic Nuclei (AGNs; see review in Hauser and Dwek [2001]), a ...

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The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe

The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe

... unobscured star-forming galaxies was determined empirically using two independent approaches to estimate the dust obscuration in the rest-frame visual band, A V ...declining star formation ...

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Unveiling the Physical Conditions in Star-Forming Galaxies at the Peak of Galaxy Assembly

Unveiling the Physical Conditions in Star-Forming Galaxies at the Peak of Galaxy Assembly

... of star formation his- tory in determining galaxy scaling relations requires data for galaxies spanning the full range of plausible star formation histories at a given ...Evolved galaxies with ...

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Star-forming galaxies as tools for cosmology in new-generation spectroscopic surveys

Star-forming galaxies as tools for cosmology in new-generation spectroscopic surveys

... model galaxies to match the observed CMASS red/blue fraction and, by consequence, it assigns each mock a specific ...bluer star-forming galaxies have lower bias, lower v pec values, lower ...

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Physical Conditions of the Interstellar Medium in Star-forming Galaxies at z~1.5

Physical Conditions of the Interstellar Medium in Star-forming Galaxies at z~1.5

... in galaxies at z ∼ ...individual galaxies, both of which are widely used as star formation indicators ...and star-forming galaxies in the local ...on star-forming ...

23

The Kiloparsec Scale Structure and Kinematics of High Redshift Star Forming Galaxies

The Kiloparsec Scale Structure and Kinematics of High Redshift Star Forming Galaxies

... actively star-forming galaxies, this is perhaps not surprising since young massive stars tend to dominate the SED out to at least rest-frame blue ...the galaxies have consistent colors, and 2) ...

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The growth of the central region by acquisition of counterrotating gas in star forming galaxies

The growth of the central region by acquisition of counterrotating gas in star forming galaxies

... ongoing star formation in growing the central region, we introduce the star formation activity parameter 21 as a SF ¼ 1/(sSFR (t H (z) 1 Gyr)), where t H (z) is the Hubble time at the redshift of the ...

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IROCKS: Spatially Resolved Kinematics of z ~ 1 Star-forming Galaxies

IROCKS: Spatially Resolved Kinematics of z ~ 1 Star-forming Galaxies

... ∼1.4 star-forming galaxies. All galaxies were observed with OSIRIS with the laser guide star adaptive optics system at Keck ...in star-forming galaxies on ...

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A correlation between star formation rate and average black hole accretion in star-forming galaxies.

A correlation between star formation rate and average black hole accretion in star-forming galaxies.

... of star-forming galaxies with SFR measurements without contam- ination from AGNs using ...for star-forming galaxies without direct X-ray ...of galaxies requires informa- ...

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Does the evolution of the radio luminosity function of star-forming galaxies match that of the star-formation rate function?

Does the evolution of the radio luminosity function of star-forming galaxies match that of the star-formation rate function?

... and star formation rate (SFR) is of crucial importance to make reliable predictions for the forthcoming ultra- deep radio surveys and to allow a full exploitation of their results to measure the cosmic star ...

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Clash: a census of magnified star-forming galaxies at z &#8764; 6-8

Clash: a census of magnified star-forming galaxies at z &#8764; 6-8

... magnified star-forming galaxies at z ∼ 6–8 presented to date, is unique in that we have observations in four WFC3/UVIS UV, seven ACS/WFC optical, and all five WFC3/IR broadband filters, which enable ...

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The redshift distribution and dust properties of dusty star-forming galaxies at high redshift

The redshift distribution and dust properties of dusty star-forming galaxies at high redshift

... dusty galaxies were a thousand times more abundant in the early Universe than they are at present ...dusty star-forming galaxies (DSFGs) were discovered in 1998, and surveys of these suggested ...

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Spitzer imaging of strongly lensed Herschel-selected dusty star-forming galaxies

Spitzer imaging of strongly lensed Herschel-selected dusty star-forming galaxies

... mass, star formation rate, visual extinction, and other parameters for each of these Herschel-selected ...and star formation rates of around 100 M e yr −1 ...normal star-forming ...

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