[PDF] Top 20 Kiloparsec-scale simulations of star formation in disk galaxies. I. the unmagnetized and zero-feedback limit
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Kiloparsec-scale simulations of star formation in disk galaxies. I. the unmagnetized and zero-feedback limit
... localized feedback from newborn stars in order to make the overall star formation rate relatively slow and inefficient at just a few percent conversion of gas to stars per local dynamical timescale ... See full document
14
Kiloparsec-Scale Simulations of star formations in disk galaxies. III. Structure and dynamics of filaments and clumps in giant molecular clouds
... the formation of dense fi laments and clumps to higher spatial resolution, ...Paper I, namely, pure hydro- dynamics of self-gravitating gas ( magnetic fi elds at this resolution and stellar feedback ... See full document
24
Spatially Resolved Star Formation in Cosmological Zoom-in Simulations: Understanding the Role of Feedback in Scaling Relations
... of star formation in the simulations, it hides the chaotic, incoherent nature of star formation on ...the simulations, the SFR is on average higher in the centers of ... See full document
187
Photoionising feedback and the star formation rates in galaxies
... the star formation simulations of Bonnell et ...small scale star formation processes as well as the large scale evolution of the interstellar medium on galactic ...Three ... See full document
10
The Kiloparsec Scale Structure and Kinematics of High Redshift Star Forming Galaxies
... guide star adaptive optics (LGSAO). We show kinematic maps of 3 target galaxies Q1623-BX453, Q0449-BX93, and DSF2237a-C2 located at redshifts z = ...rotating disk of ionized gas as the local velocity ... See full document
250
Kiloparsec-scale Simulations of Star Formation in Disk Galaxies. IV. Regulation of Galactic Star Formation Rates by Stellar Feedback
... the kiloparsec-scale patch down to much higher resolution (∼ ...Myr. Star formation was included with the same recipe as in Papers I and II, but now with a higher density threshold of n ... See full document
24
Star formation histories of z~1 galaxies in LEGA C
... for galaxies at z ∼ ...in star formation); using a defined set of template spectra which allow for di- rect comparisons of the SFHs; as well as the assumption of constant star formation ... See full document
18
Bulgeless galaxies in the COSMOS field:environment and star formation evolution at z
... bulgeless galaxies within the current picture of galaxy formation and evo- lution, Bizzocchi et ...evolved galaxies (from early-type spirals to lenticulars and ...either star-formation ... See full document
14
What governs star formation in galaxies? A modern statistical approach
... of galaxies such as morphology and dust mass have been tested as well, but there is no SFR law that considers all of the above quantities ...empirical star formation law, suggesting that SFR and ... See full document
150
Eisenreich, Maximilian (2018): Supermassive black holes and multiphase gas in early-type galaxies. Dissertation, LMU München: Fakultät für Physik
... the star-formation and subsequent stellar feedback in the cold, dense disc and core raises the metallicity in the centre up to two to three times the solar value, but the constant inflow of gas from ... See full document
195
Near ultraviolet signatures of environment driven galaxy quenching in Sloan Digital Sky Survey groups
... all galaxies in the matched ...sequence galaxies with a large red population, and a blue ...sequence galaxies with (NUV − r) < ...of galaxies with residual are formation from NUV ... See full document
12
Morphology and the color mass diagram as clues to galaxy evolution at z∼1
... of star formation in galaxies at z ∼ 1, by examining their color-mass distributions for different morphology ...∼5,000 galaxies and X-ray selected active galactic nucleus (AGN) hosts in the ... See full document
12
Pannella, Maurilio (2007): Morphological evolution of galaxies over the last 8 billion years. Dissertation, LMU München: Fakultät für Physik
... and star formation activity as a function of morphology and ...late–type galaxies in the stellar mass ...type galaxies fall in between, confirming their nature of transition ...mass: ... See full document
179
The energetics of starburst driven outflows at z ∼ 1 from KMOS
... examine galaxies observed as part of the ...743 star-forming galaxies at z ∼ 1 selected from some of the best studies extra-galactic survey fields (ECDFS, COSMOS, UDS and SSA ...the galaxies ... See full document
15
The SAMI Galaxy Survey : spatially resolving the environmental quenching of star formation in GAMA galaxies
... for galaxies with a range of stellar masses and star-forming morphologies in ...201 star-forming galaxies in the sample resulted in the identification of 15 galaxies where the galaxy ... See full document
22
Regulation of Star Formation Amidst Heating and Cooling in Galaxies and Galaxy Clusters
... of feedback mainly operates at low ...of feedback, mechanical energy released by an AGN in the form of jets is responsible for heating and increasing the cooling time at the center of massive ...inhibits ... See full document
198
A New Method to Measure and Map the Gas Scale Height of Disk Galaxies
... gas scale height of galactic disks is an important quantity related to the process of star ...between star formation processes and gravity, and the interstellar medium pressure, which must be ... See full document
5
Gravitational transformation of gaseous clouds: The formation of spiral galaxies and disk planets
... in formation of natural systems like galaxies and ...its disk are simulated using a novel N-body self-gravi- tational ...and disk of the planet is the result of gravitational contrac- tion of ... See full document
20
Fossati, Matteo (2016): Environmentally driven suppression of star formation in galaxies over the last 10 billion years. Dissertation, LMU München: Fakultät für Physik
... passive galaxies as a function of halo mass and stellar mass) predicted by the ...central galaxies is far from being linear or independent of stellar mass, the passive fraction depends both on density and ... See full document
208
SDSS IV MaNGA resolved star formation and molecular gas properties of green valley galaxies: a first look with ALMA and MaNGA
... three galaxies represent a sequence of transitional stages, our results would favor an inside-out quenching — the SF is ceased in the bulge fi rst because of the lack of available cold gas, followed by the ... See full document
9
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