ORBITS, DISTANCE, AND STELLAR MASSES OF THE MASSIVE TRIPLE STAR σ ORIONIS [PDF]
We present interferometric observations of the σ Orionis triple system using the CHARA Array, NPOI, and VLTI. Using these measurements, we spatially resolve the orbit of the close spectroscopic binary (Aa,Ab) for the first time and present a revised ...
G. Schaefer +13 more
semanticscholar +1 more source
Radio observations of stellar mass loss [PDF]
A program to search for steady-state thermal emissions from stars has been in progress for several years in Canada (Purton 1976). In this program we have specifically excluded flaring objects (such as β Lyr or HR1099) where non-thermal emission is probably responsible.
Sun Kwok, C. R. Purton
openaire +1 more source
The luminosity and stellar mass Fundamental Plane of early-type galaxies [PDF]
From a sample of ~50000 early-type galaxies from the SDSS, we measured the traditional Fundamental Plane in four bands. We then replaced luminosity with stellar mass, and measured the "stellar mass" FP.
Bell +40 more
core +3 more sources
STELLAR MASSES AND STAR FORMATION RATES FOR 1 M GALAXIES FROM SDSS+WISE [PDF]
We combine Sloan Digitital Sky Survey (SDSS) and WISE photometry for the full SDSS spectroscopic galaxy sample, creating spectral energy distributions (SEDs) that cover λ = 0.4–22 μm for an unprecedentedly large and comprehensive sample of 858,365 ...
Yu-Yen Chang +3 more
semanticscholar +1 more source
Benchmarking pre-main sequence stellar evolutionary tracks using disk-based dynamical stellar masses
Stellar masses are a fundamental property to understand models of pre-main sequence evolution, but their values derived from Hertzsprung–Russell (HR) diagrams are strongly model dependent.
Zallio Luigi +16 more
doaj +1 more source
Breaking down the link between luminous and dark matter in massive galaxies
We present a study on the clustering of a stellar mass selected sample of galaxies with stellar masses M*>10^10Msol at redshifts 0 ...
Christopher J. Conselice +4 more
core +1 more source
THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G): STELLAR MASSES, SIZES, AND RADIAL PROFILES FOR 2352 NEARBY GALAXIES [PDF]
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey of 2352 nearby galaxies with deep imaging at 3.6 and 4.5 μm.
J. Muńoz-Mateos +27 more
semanticscholar +1 more source
[Abridged] We present optical and NIR observations of 19 short GRB host galaxies, aimed at measuring their stellar masses and population ages. The goals of this study are to evaluate whether short GRBs track the stellar mass distribution of galaxies, to ...
Belczynski +36 more
core +1 more source
The masses and metallicities of stellar haloes reflect galactic merger histories [PDF]
There is increasing observational and theoretical evidence for a correlation between the metallicity and the mass of the stellar halo for galaxies with Milky Way-like stellar masses.
R. D’Souza, E. Bell
semanticscholar +1 more source
The California-Kepler Survey. II. Precise Physical Properties of 2025 Kepler Planets and Their Host Stars [PDF]
We present stellar and planetary properties for 1305 Kepler Objects of Interest (KOIs) hosting 2025 planet candidates observed as part of the California-Kepler Survey.
Cargile, Phillip A. +13 more
core +3 more sources

