STELLAR MASSES
Resolved millimeter dust continuum cavity around the very low mass young star CIDA 1
... its stellar mass, as shown in the left panel of ...the stellar masses calculated using the evolu- tionary models of Baraffe et ...dust masses obtained in Andrews et ...
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The different star formation histories of blue and red spiral and elliptical galaxies
... of stellar masses for the six samples in ...low stellar masses, which explains this trend – note that red early-type spirals are on average slightly more massive than blue early-type ...of ...
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The cosmic web unravelled : a study of filamentary structure in the Galaxy and Mass Assembly survey
... All three equatorial regions are more than 98% spectroscopically complete (Driver et al., 2011), and the two southern fields are in the process of being completed. GAMA has been designed to have over 1000 objects per ...
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Galaxy And Mass Assembly (GAMA) : stellar mass growth of spiral galaxies in the cosmic web
... in stellar mass and star formation rate (SFR) along filaments in the cosmic web by examining the stellar masses and UV-derived SFRs of 1799 ungrouped and unpaired spiral galaxies that reside in ...
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The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
... highest masses. Of course the only direct means of establishing stellar masses is via close ...dynamical masses of a few systems, although spec- troscopic and photometric searches for other ...
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The SAMI Galaxy Survey : spatially resolving the main sequence of star formation
... We begin by comparing the integrated properties of SAMI galaxies to the global SFMS. We sum the SFR maps for each galaxy to obtain the total SFR and use the total stellar masses from the GAMA catalogue. ...
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Galaxy And Mass Assembly (GAMA) : testing galaxy formation models through the most massive galaxies in the Universe
... BCG stellar mass since z = ...BCG stellar masses 9 billion years ago were not very different to their stellar masses now (Aragon-Salamanca, Baugh & Kauffmann 1998; Baugh et ...
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The dependence of galaxy clustering on stellar mass, star formation rate and redshift at z = 0 8 − 2 2, with HiZELS
... our stellar masses, especially in SA22 where fewer bands are available, we compare our stellar mass estimates to apparent K-band luminosities, which broadly trace the older stellar population ...
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GAMA/G10 COSMOS/3D HST : the 0 < z < 5 cosmic star formation history, stellar and dust mass densities
... our stellar mass coverage to the very dis- tant Universe we also include the 3D-HST dataset (Mom- cheva et ...include stellar mass estimates based on SED fitting under the assumption of a Kroupa (2001) IMF ...
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Galaxy Zoo: morphological classification of galaxy images from the Illustris simulation
... Modern large-scale cosmological simulations model the universe with increasing sophistication and at higher spatial and temporal resolutions. These ongoing enhancements permit increasingly detailed comparisons between ...
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A distance-limited sample of massive star-forming cores from the RMS Survey
... Figure 14. Mass-luminosity plot for all MYSOs and Hii regions, with mass flags 0 and 1 as circles, flag 2 sources as squares and flag 4 sources as triangles. Open and filled symbols separate MYSOs and Hii regions. The ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) : galaxy segregation inside filaments at z ≃ 0 7
... different stellar masses and stellar activities are distributed around the filaments and find a significant segregation, with the most massive or quiescent galaxies being closer to the filament axis ...
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Galaxy And Mass Assembly (GAMA) : the environments of high and low excitation radio galaxies
... The stellar masses used in this work are larger than those estimated using KCORRECT , which is caused by the different types of photom- etry [Taylor et ...the stellar masses is to generate ...
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P MaNGA : full spectral fitting and stellar population maps from prototype observations
... those output of the SDSS-III/BOSS data release and pipeline (Daw- son et al. 2013). In brief, these are also broad band ugriz SED fitting performed with the publicly available code Hyper-Z customed with Maraston (2005) ...
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SDSS IV MaNGA: star formation cessation in low redshift galaxies I: dependence on stellar mass and structural properties
... galaxies in the class of SF or PQ, which have small B / T luminosity ratios. We note that this trend might be driven by the lack of SF spheroid-like galaxies. However, given the small number of SF spheroid-like galaxies ...
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On the M σ Relationship and SMBH Mass Estimates of Selected Nearby Galaxies
... SMBH masses and determined upper and lower mass bounda- ries and the mass histogram for spiral galaxies in a narrow redshift regime ...estimating stellar bulge velocity dispersion and estimated the central ...
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The Atlas3D Project XXX Star formation histories and stellar population scaling relations of early type galaxies
... case. This criterion is suggested by Press et al. (1992) as a robust indication of when the fit has become unacceptable. In this way, we are deriving the smoothest SFH that still reproduces the SAURON spectrum. The ...
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Galaxy and Mass Assembly (GAMA) : halo formation times and halo assembly bias on the cosmic web
... or stellar mass (massive galaxies are more common in denser regions) are accounted for, most authors find no significant effect of the GE on the galaxy or halo ...for stellar mass, Alpaslan et ...by ...
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Accretion discs as regulators of stellar angular momentum evolution in the ONC and Taurus Auriga
... the stellar mass in solar units and the age in Myr, estimated from T eff and log (L / L ) using Siess et ...the stellar radius in solar units; column 13 lists the rotation period in days; column 14 lists ...
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The Shapes of the Rotation Curves of Star forming Galaxies Over the Last ~10 Gyr
... the stellar-scaled scaling prescription, we stacked deep MUSE and KMOS observations of the spatially-resolved nebular emission from ≈1500 star-forming galaxies between z ≈ ...redshift, stellar mass, and ...
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