Results 11 to 20 of about 74,495 (201)

The Eclipsing Binaries from the LAMOST Medium-resolution Survey. III. A High-precision Empirical Stellar Mass Library

open access: yesThe Astronomical Journal, 2023
High-precision stellar masses and radii measured directly from binaries can effectively calibrate stellar models. However, such a database containing full spectral types and a large range of metallicity is still not fully established. A continuous effort
Jianping Xiong   +8 more
doaj   +1 more source

A collection of model stellar spectra for spectral types B to early-M [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Models of stellar spectra are necessary for interpreting light from individual stars, planets, integrated stellar populations, nebulae, and the interstellar medium.Aims. We provide a comprehensive and homogeneous collection of synthetic spectra for a wide range of atmospheric parameters and chemical compositions.Methods.
Prieto, Carlos Allende   +5 more
openaire   +2 more sources

Spectral Classification of Galaxies Along the Hubble Sequence [PDF]

open access: yes, 1995
We develop a straightforward and quantitative two-step method for spectroscopically classifying galaxies from the low signal-to-noise (S/N) optical spectra typical of galaxy redshift surveys. First, using \chi^2-fitting of characteristic templates to the
Willick, Jeffrey A.   +2 more
core   +2 more sources

The Spitzer Atlas of Stellar Spectra [PDF]

open access: yes, 2010
We present the Spitzer Atlas of Stellar Spectra (SASS), which includes 159 stellar spectra (5 to 32 mic; R~100) taken with the Infrared Spectrograph on the Spitzer Space Telescope.
D. W. Hoard   +9 more
core   +2 more sources

SPECTRAL TYPING OF LATE-TYPE STELLAR COMPANIONS TO YOUNG STARS FROM LOW-DISPERSION NEAR-INFRARED INTEGRAL FIELD UNIT DATA [PDF]

open access: yesThe Astronomical Journal, 2012
We used the Project 1640 near-infrared coronagraph and integral field spectrograph to observe 19 young solar type stars. Five of these stars are known binary stars and we detected the late-type secondaries and were able to measure their JH spectra with a resolution of R\sim30.
Roberts, Lewis C., Jr.   +24 more
openaire   +3 more sources

Magellanic System Stars Identified in SMACS J0723.3-7327 James Webb Space Telescope Early Release Observations Images

open access: yesThe Astrophysical Journal, 2023
We identify 71 distant stars in James Webb Space Telescope/NIRCam early release observations (ERO) images of the field of galaxy cluster SMACS J0723.3-7327 (SMACS 0723).
Jake Summers   +25 more
doaj   +1 more source

Stellar Chromospheric Variability

open access: yesUniverse, 2021
Cool stars with convective envelopes of spectral types F and later tend to exhibit magnetic activity throughout their atmospheres. The presence of strong and variable magnetic fields is evidenced by photospheric starspots, chromospheric plages and ...
Richard de Grijs, Devika Kamath
doaj   +1 more source

Evaluating GAIA performances on eclipsing binaries. I. Orbits and stellar parameters for V505 Per, V570 Per and OO Peg [PDF]

open access: yes, 2001
The orbits and physical parameters of three detached, double-lined A-F eclipsing binaries have been derived combining H_P, V_T, B_T photometry from the Hipparcos/Tycho mission with 8500-8750 Ang ground-based spectroscopy, mimicking the photometric ...
A. Prša   +26 more
core   +4 more sources

New X-ray Selected Pre-Main Sequence Members of the Serpens Molecular Cloud [PDF]

open access: yes, 2013
The study of young stars no longer surrounded by disks can greatly add to our understanding of how protoplanetary disks evolve and planets form. We have used VLT/FLAMES optical spectroscopy to confirm the youth and membership of 19 new young diskless ...
Brown, Joanna M.   +2 more
core   +2 more sources

The Nature of Blue Stars with Mid-infrared Excesses in the Large Magellanic Cloud

open access: yesThe Astrophysical Journal Supplement Series, 2023
We present low-resolution optical spectra and classifications of 92 blue objects with mid-infrared excesses in the Large Magellanic Cloud. The majority of these objects were selected with the criteria of U − B < 0 and V < 17 from the potential young ...
Ryoko Ishioka   +5 more
doaj   +1 more source

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