Results 31 to 40 of about 2,699,264 (331)
The Carnegie-Irvine Galaxy Survey. X. Bulges in Stellar Mass–based Scaling Relations
We measure optical colors for the bulges of 312 disk galaxies from the Carnegie-Irvine Galaxy Survey and convert their previously available R -band structural parameters to stellar-mass parameters.
Hua Gao, Luis C. Ho, Zhao-Yu Li
doaj +1 more source
Application of convolutional neural networks for stellar spectral classification [PDF]
Due to the ever-expanding volume of observed spectroscopic data from surveys such as SDSS and LAMOST, it has become important to apply artificial intelligence (AI) techniques for analysing stellar spectra to solve spectral classification and regression
K. Sharma +5 more
semanticscholar +1 more source
CLASSIFICATION OF STELLAR ORBITS IN AXISYMMETRIC GALAXIES [PDF]
7 pages, 9 figures and 1 table. Submitted to ApJ.
Baile Li +2 more
openaire +2 more sources
Classification of Stellar Spectra [PDF]
SummaryThe objectives of this exercise are to gain familiarity with the appearance of the spectra of stars, to understand some of the temperature and luminosity criteria used to classify spectra, and to gain insights into the relationship between the appearance of stellar spectra and physical conditions in stellar atmospheres.
openaire +1 more source
Automatic Extraction and Classification of Low-Dispersion Objective-Prism Stellar Spectra
An automatic method of spectral classification from low-dispersion objective prism images is developed. The distribution of early- and late-type stars inside stellar complexes and their surrounding regions can lead to important clues on the star ...
Bratsolis E. +5 more
doaj +3 more sources
The year 1943 saw the introduction of the Morgan-Keenan (MK) classification scheme and this replaced the existing Harvard Classification scheme. Both stellar classification scheme are fundamentally grounded in the field of spectroscopy.
Magee, John
core +1 more source
The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
The goal of AMBRE, a joint project between ESO and the Observatoire de la Cote d’Azur, is to provide a homogeneous determination of the stellar parameters (including mean metallicity and some chemical abundances) for the archived spectra of the FEROS ...
Hill V. +4 more
doaj +1 more source
POSYDON: A General-purpose Population Synthesis Code with Detailed Binary-evolution Simulations
Most massive stars are members of a binary or a higher-order stellar system, where the presence of a binary companion can decisively alter their evolution via binary interactions. Interacting binaries are also important astrophysical laboratories for the
Tassos Fragos +24 more
doaj +1 more source
Commission 45: Stellar Classification: (Classification Stellaire) [PDF]
This report does not intend to give a complete review of all the papers that appeared since the previous General Assembly but to focus on a few subjects only.
Michèle Gerbaldi +10 more
openaire +1 more source
Architecture of Hierarchical Stellar Systems and Their Formation
Accumulation of new data on stellar hierarchical systems and the progress in numerical simulations of their formation open the door to genetic classification of these systems, where properties of a certain group (family) of objects are tentatively ...
Andrei Tokovinin
core +1 more source

