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STAR-FORMATION RATE

The mean star formation rate of X ray selected active galaxies and its evolution from z ~ 2 5: Results from PEP Herschel

The mean star formation rate of X ray selected active galaxies and its evolution from z ~ 2 5: Results from PEP Herschel

... host star- formation and AGN activity are an essential test of the de- gree and importance of galaxy-SMBH co-evolution ...of star-formation in AGNs have con- centrated on interesting ...

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A Chandra Perspective on Galaxy Wide X ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxies

A Chandra Perspective on Galaxy Wide X ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxies

... nents that were undetected in the 2–8 keV band. For NGC 23, the nucleus was detected in the 2–8 keV band, but due to the increased background over the larger galaxy-wide area, the total galaxy emission was formally ...

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Disentangling the Galactic Halo with APOGEE  II  Chemical and Star Formation Histories for the Two Distinct Populations

Disentangling the Galactic Halo with APOGEE II Chemical and Star Formation Histories for the Two Distinct Populations

... The formation processes that led to the current Galactic stellar halo are still under ...and star formation histories ( SFHs ) ...the star formation rate, and its duration for ...

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The lack of star formation gradients in galaxy groups up to z ~ 1 6

The lack of star formation gradients in galaxy groups up to z ~ 1 6

... generally star forming, and early-type galaxies passive, this implies a possible relationship between star formation rate (SFR) and density, and a number of studies have focused on this ...

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Star formation in AGN hosts in GOODS N

Star formation in AGN hosts in GOODS N

... the star formation rate of the host galaxy is important for studying the co-evolution of active galactic nuclei (AGN) and their ...host star formation rate diagnostic of high-z ...

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Galaxy evolution: A new version of the Besançon Galaxy Model constrained with Tycho data

Galaxy evolution: A new version of the Besançon Galaxy Model constrained with Tycho data

... the star produc- tion process in that model was based on the drawing from the so called Hess ...(IMF), Star Formation Rate (SFR), evolutionary tracks and age-metallicity relation and since ...

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Large scale modulation of star formation in void walls

Large scale modulation of star formation in void walls

... of star formation in the galaxy, which allows to define a spectral ...specific star formation rate in galaxies becomes higher as η ...the star formation activity ...

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LLAMA: normal star formation efficiencies of molecular gas in the centres of luminous Seyfert galaxies

LLAMA: normal star formation efficiencies of molecular gas in the centres of luminous Seyfert galaxies

... the star formation rate (SFR) within galaxies (Bigiel et ...in star-forming galax- ies (Leroy et ...the star-formation associated with the gas ...‘star formation ...

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Converting H alpha luminosities into star formation rates

Converting H alpha luminosities into star formation rates

... of star formation, galactic evolu- tion, and ...current star formation rates ...massive star formation ...sive star formation to total star formation ...

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Infrared Emission from the Nearby Cool Core Cluster Abell 2597

Infrared Emission from the Nearby Cool Core Cluster Abell 2597

... IR-inferred star formation rate is also consistent with the conclusion of O’Dea et ...the rate of a few solar masses per year, are the dominant source of ion- ization of the optical ...

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A possible origin of the mass metallicity relation of galaxies

A possible origin of the mass metallicity relation of galaxies

... current star formation rate have been found to contain star clusters up to a lower mass ...low star formation, the stellar initial mass function does not extend to as high masses ...

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Ly alpha emission line galaxies at z=3 1 in the extended Chandra Deep Field South

Ly alpha emission line galaxies at z=3 1 in the extended Chandra Deep Field South

... Since Ly galaxies have been observed at a number of red- shifts, it is tempting to use our data to examine the evolution of the LAE luminosity function. Unfortunately, the samples ob- tained to date are not yet robust ...

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The ACS Virgo Cluster Survey  XV  The Formation Efficiencies of Globular Clusters in Early Type Galaxies: The Effects of Mass and Environment

The ACS Virgo Cluster Survey XV The Formation Efficiencies of Globular Clusters in Early Type Galaxies: The Effects of Mass and Environment

... peak star formation rates and densities) in order to have more of their stars in massive ...normalized star formation rate of early-type cluster dwarfs as a function of look-back ...The ...

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Recent Galaxy Mergers and Residual Star Formation of Red Sequence Galaxies in Galaxy Clusters

Recent Galaxy Mergers and Residual Star Formation of Red Sequence Galaxies in Galaxy Clusters

... Although the RSF fraction of post-merger galaxies seemed larger than that of normal galaxies, only 30% ( 21 / 70 ) of RSF galaxies among the optical red sequence galaxies showed post- merger signatures in the deep ...

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STAR

STAR

... de STAR y sus pretensiones revolucionarias, habría que remover la historia – promovida a día de hoy por aquellos a quienes les gustaría evitar la necesidad de la lucha en sus vidas actuales – de Stonewall como el ...

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Panchromatic estimation of star formation rates in BzK galaxies at 1 <z< 3

Panchromatic estimation of star formation rates in BzK galaxies at 1 <z< 3

... Notes. Star formation rates for redshift-binned sBzKs. Column 1: sample redshift range; Column 2: SFR from integrated IR luminosity using CE01 template fits to MIR–radio photometry (λ 24 μm); Column 3: SFR ...

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Simulations of star formation in a gaseous disc around Sgr A*  a failed Active Galactic Nucleus

Simulations of star formation in a gaseous disc around Sgr A* a failed Active Galactic Nucleus

... simulate star formation in an accretion disc around Sgr A ∗ in the low disc mass ...accretion rate of stars to a fraction of the Eddington ...

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TIDAL DISRUPTIONS IN CIRCUMBINARY DISKS  I  STAR FORMATION, DYNAMICS, AND BINARY EVOLUTION

TIDAL DISRUPTIONS IN CIRCUMBINARY DISKS I STAR FORMATION, DYNAMICS, AND BINARY EVOLUTION

... The early dynamical evolution (first few hundred Ω − 0 1 ) is dominated by close encounters between the MBH binary and stars on radial orbits (i.e., in the loss cone of the binary). This is naturally accompanied by a ...

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Multiwavelength Study of Massive Galaxies at z~2  I  Star Formation and Galaxy Growth

Multiwavelength Study of Massive Galaxies at z~2 I Star Formation and Galaxy Growth

... various star formation tracers persists in- dividually for distant massive galaxies, hence to what extent SFRs can be unambiguously measured at high ...actively star- forming galaxies ( Noeske et ...

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Ly alpha emitting galaxies at z=3 1: L* progenitors experiencing rapid star formation

Ly alpha emitting galaxies at z=3 1: L* progenitors experiencing rapid star formation

... success rate for the slit- masks with the highest S/N was 90%, setting an upper limit of 10% on possible contamination of our LAE ...The rate of non-detections was higher in masks with shorter exposure ...

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