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Comparison of Stellar Masses Derived from CB07 and BC03 models

Stellar masses of SDSS-III/BOSS galaxies at z ~ 0.5 and constraints to galaxy formation models

Stellar masses of SDSS-III/BOSS galaxies at z ~ 0.5 and constraints to galaxy formation models

... data-derived stellar masses reflect the ±1σ vari- ation in stellar mass according to the χ 2 of the ...empirical stellar mass function were estimated by combin- ing in quadrature the ...

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The luminosity functions and stellar masses of galactic disks and spheroids.

The luminosity functions and stellar masses of galactic disks and spheroids.

... photometric comparison technique to esti- mate the B-band bulge-to-disk ratios of ...the stellar mass ...who derived a ratio of disk to spheroid stellar mass density of 0:33  ...the ...

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Red giant masses and ages derived from carbon and nitrogen abundances

Red giant masses and ages derived from carbon and nitrogen abundances

... determine stellar masses and ages that can be applied to large numbers of stars over a large volume of the ...APOGEE stellar spectra of giant stars to derive their masses and ...of ...

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The Spitzer Survey of Stellar Structure in Galaxies (S^4G): Stellar Masses, Sizes, and Radial Profiles for 2352 nearby Galaxies

The Spitzer Survey of Stellar Structure in Galaxies (S^4G): Stellar Masses, Sizes, and Radial Profiles for 2352 nearby Galaxies

... of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey of 2352 nearby galaxies with deep imaging at ...central stellar mass concentration for galaxies with the same total ...

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Comparing dynamical and photometric-stellar masses of early-type galaxies at z ~ 1

Comparing dynamical and photometric-stellar masses of early-type galaxies at z ~ 1

... collected from ground-based and space- based observatories has enabled the measurement of stellar masses by fitting widely-sampled spectral energy distri- butions (SED) of galaxies with spectrum ...

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A comparison of simulated JWST observations derived from equilibrium and non equilibrium chemistry models of giant exoplanets

A comparison of simulated JWST observations derived from equilibrium and non equilibrium chemistry models of giant exoplanets

... planetary masses and equilibrium temperatures, from hot and Jupiter-sized to warm and ...model from Venot et ...differences from 4 to 5 µ m due to disequilibrium from CO and CO 2 ...

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Stellar masses and disk properties of Lupus young stellar objects traced by velocity-aligned stacked ALMA 13CO and C18O spectra

Stellar masses and disk properties of Lupus young stellar objects traced by velocity-aligned stacked ALMA 13CO and C18O spectra

... disk models The model disks were made with two intensity distributions, uni- form and Gaussian distributions, two stellar masses, ...respectively. From those, model image cubes were produced ...

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From K giants to G dwarfs: stellar lifetime effects on metallicity distributions derived from red giants

From K giants to G dwarfs: stellar lifetime effects on metallicity distributions derived from red giants

... current models. While the need to account for vari- able stellar lifetimes was appreciated very early on in the integrated light study of galaxy spectra ...inferences from samples of individually ...

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Comparing ROC Curves Derived From Regression Models

Comparing ROC Curves Derived From Regression Models

... of the markers and instead constructs predictors to maximize the likelihood. In most cases this results in an optimized ROC curve. Consequently both ROC curves are optimized in the same direction. Both of these phenomena ...

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Study of visualizations for n-body stellar models

Study of visualizations for n-body stellar models

... Overview Stellar modeling on the galactic level involves calculation of the n-body ...positions, masses, and ...made from the raw ...For stellar models this could be information such as ...

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Stellar magnetism and activity :  from stellar interiors to orbiting exoplanets

Stellar magnetism and activity : from stellar interiors to orbiting exoplanets

... both models, can be found in Table ...of stellar mass, each at a constant chromospheric ...the models presented in ...the stellar masses present in the Bcool ...

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Clues from stellar catastrophes

Clues from stellar catastrophes

... to models of quiescent galactic nuclei in Chapter 3, where we outline ‘autarkic’ or self-similar dependences of properties of the gas and stellar population on the SMBH ...found from our code, for ...

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A comparison of optical and near-infrared colours of Magellanic Cloud star clusters with predictions of simple stellar population models

A comparison of optical and near-infrared colours of Magellanic Cloud star clusters with predictions of simple stellar population models

... age from ≈200 Myr to >10 Gyr, and have [Fe/H] values from ...simple stellar population models in the optical/near-infrared (near-IR) colour–colour ...accumulated masses for most ...

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Comparison of the pathogen species-specific immune response in udder derived cell types and their models

Comparison of the pathogen species-specific immune response in udder derived cell types and their models

... Discussion The udder is composed of a variety of different cell types each featuring a developmentally determined distinct immune competence. Their interplay governs the patho- gen species-specific immune physiology of ...

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Understanding the effects of stellar multiplicity on the derived planet radii from transit surveys: implications for Kepler, K2, and TESS

Understanding the effects of stellar multiplicity on the derived planet radii from transit surveys: implications for Kepler, K2, and TESS

... include stellar spectroscopy, a few radial velocity measurements, and ...potential stellar companions with orbital periods of ≲ 1 –2 yr or ...and stellar masses for any stellar ...

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Constraining stellar physics from red-giant stars in binaries – stellar rotation, mixing processes and stellar activity

Constraining stellar physics from red-giant stars in binaries – stellar rotation, mixing processes and stellar activity

... in Stellar Pa- rameters (gssp 1 ) software package by ...ratio derived from the solution of spectral disentangling indi- cates that the masses of the two stars is very similar the ...

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Determination and comparison rate of expression markers of osteoblast derived of Adipose derived stem cells markers in monolayer and pellet culture models

Determination and comparison rate of expression markers of osteoblast derived of Adipose derived stem cells markers in monolayer and pellet culture models

... extracted from the cells using RNAx -plus solution (CinnaGen Inc ...prepared from 1µg the total RNA using oligo(dt)18 as a primer and Revert Aid TM First-strand cDNA synthesis kit (Fermentase) according to ...

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Star formation and stellar mass assembly in galaxy formation models

Star formation and stellar mass assembly in galaxy formation models

... baryons from satellite galaxies are instantly merged onto the central galaxy upon subhalo ...the stellar mass assembly history of the central ...of comparison, we choose to also show the evolutionary ...

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Thomas, Jens
  

(2006):


	The distribution of dark matter and stellar orbits in nine Coma early-type galaxies derived from their stellar kinematics.


Dissertation, LMU München: Fakultät für Physik

Thomas, Jens (2006): The distribution of dark matter and stellar orbits in nine Coma early-type galaxies derived from their stellar kinematics. Dissertation, LMU München: Fakultät für Physik

... the stellar population ages implied by the SSP models devote some further ...SSP models is gas emission, which refills the stellar Hβ absorption ...resulting stellar populations are ...

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Policy Advice Derived From Simulation Models

Policy Advice Derived From Simulation Models

... infer from empirical facts and observations to the general patterns underlying them, thereby giving a causal explanation on a deeper level and distinguishing chance from structural ...cover models ...

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