about
Early turbulent mixing as the origin of chemical homogeneity in open star clusters.The formation of massive star systems by accretion.Molecular hydrogen deficiency in H I-poor galaxies and its implications for star formationVery Massive Stars in the local UniverseSteady outflows in giant clumps of high-z disc galaxies during migration and growth by accretionThe role of stellar feedback in the dynamics of H II regionsThe big problems in star formation: The star formation rate, stellar clustering, and the initial mass functionThe chemical signatures of the first star clusters in the universeMetallicity fluctuation statistics in the interstellar medium and young stars – I. Variance and correlationInflow of atomic gas fuelling star formationMassive stars formed in atomic hydrogen reservoirs: H I observations of gamma-ray burst host galaxiesLegacy extragalactic UV survey (LEGUS) with the Hubble Space Telescope. I. Survey descriptionMassive Star FormationThe brightest young star clusters in NGC 5253COLD GASS, an IRAM legacy survey of molecular gas in massive galaxies - I. Relations between H2, H i, stellar content and structural propertiesCOLD GASS, an IRAM legacy survey of molecular gas in massive galaxies - II. The non-universality of the molecular gas depletion time-scaleThe bursty star formation histories of low-mass galaxies at 0.4 < z < 1 revealed by star formation rates measured from H{beta} and FUVThe intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep FieldDense Gas, Dynamical Equilibrium Pressure, and Star Formation in Nearby Star-forming GalaxiesFull-disc ¹³CO(1–0) mapping across nearby galaxies of the EMPIRE survey and the CO-to-H₂ conversion factorSuppression of star formation in dwarf galaxies by photoelectric grain heating feedbackThe formation of stars by gravitational collapse rather than competitive accretionLegacy ExtraGalactic UV Survey with The Hubble Space Telescope: Stellar Cluster Catalogs and First Insights Into Cluster Formation and Evolution in NGC 628Extinction Maps and Dust-to-gas Ratios in Nearby Galaxies with LEGUSThe Resolved Stellar Populations in the LEGUS Galaxies1Exploring the IMF of star clusters: a joint SLUG and LEGUS effortStar cluster properties in two LEGUS galaxies computed with stochastic stellar population synthesis modelsHierarchical Star Formation in Turbulent Media: Evidence from Young Star ClustersBig fish in small ponds: massive stars in the low-mass clusters of M83Protostellar feedback in turbulent fragmentation: consequences for stellar clustering and multiplicityThe necessity of feedback physics in setting the peak of the initial mass functionThe AGORA high-resolution galaxy simulations comparison projectConverging on the Initial Mass Function of StarsAn initial mass function study of the dwarf starburst galaxy NGC 4214The art of modelling CO, [C i], and [C ii] in cosmological galaxy formation modelsDark Molecular Gas in Simulations of z ∼ 0 Disk GalaxiesA physical model for the [C ii]–FIR deficit in luminous galaxiesA theory for the excitation of CO in star-forming galaxiesA general model for the CO-H2 conversion factor in galaxies with applications to the star formation lawThe CO-H2 conversion factor in disc galaxies and mergers
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hulumtues
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researcher
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հետազոտող
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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Mark R Krumholz
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P496
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P735
P7859
lccn-no2016126205