Results 61 to 70 of about 8,488 (185)
A Multidata Approach to Open Clusters: Roslund 3 and Ruprecht 174 in CCD UBV and Gaia DR3 Context
A detailed analysis of the structural, astrophysical, kinematic, and dynamical properties of the open clusters Roslund 3 and Ruprecht 174 is carried out using CCD UBV photometry in conjunction with astrometric and photometric data from Gaia DR3 ...
Hülya Karagöz +7 more
doaj +1 more source
Fundamental parameters and infrared excesses of Hipparcos stars
We derive the fundamental parameters (temperature and luminosity) of 107 619 Hipparcos stars and place these stars on a true Hertzsprung-Russell diagram.
A. A. Zijlstra +68 more
core +1 more source
The Large Magellanic Cloud (LMC) is the Milky Way’s most massive satellite. Its interactions with the Small Magellanic Cloud are expected to leave imprints on its structure and evolution. In this work, we use the LMC outer star cluster population to seek
Bernardo P. L. Ferreira +14 more
doaj +1 more source
PANCAKE: A Python-based Numerical Color–Magnitude Diagram Analysis Package
Stellar populations serve as a fossil record of galaxy formation and evolution, providing crucial information about the history of star formation and galaxy evolution.
Yun Zheng +13 more
doaj +1 more source
Asteroseismology of red giants & galactic archaeology
Red-giant stars are low- to intermediate-mass ($M \lesssim 10$~M$_{\odot}$) stars that have exhausted hydrogen in the core. These extended, cool and hence red stars are key targets for stellar evolution studies as well as galactic studies for several ...
A. Baglin +72 more
core +1 more source
X rays from old open clusters: M 67 and NGC 188 [PDF]
We have observed the old open clusters M 67 and NGC 188 with the ROSAT PSPC. In M 67 we detect a variety of X-ray sources. The X-ray emission by a cataclysmic variable, a single hot white dwarf, two contact binaries, and some RS CVn systems is as ...
Belloni, T., Mathieu, R. D., Verbunt, F.
core +2 more sources
The Star Formation History of Nearby Galaxies: A Machine Learning Approach
Reproducing color–magnitude diagrams (CMDs) of star-resolved galaxies is one of the most precise methods for measuring the star formation history (SFH) of nearby galaxies back to the earliest time.
Yujiao Yang +4 more
doaj +1 more source
The Ages of Pre-main-sequence Stars
The position of pre-main-sequence or protostars in the Hertzsprung--Russell diagram is often used to determine their mass and age by comparison with pre-main-sequence evolution tracks.
Alexander +45 more
core +2 more sources
A comprehensive study of δ Scuti-type pulsators in eclipsing binaries: Oscillating eclipsing Algols
Eclipsing double-lined spectroscopic binaries (SB2s) hosting δ Scuti-type pulsators offer a unique laboratory for simultaneously constraining stellar geometry and interior structure.
Pawar T. +6 more
doaj +1 more source
Fundamental parameters and time-evolution of mass loss are investigated for post-main-sequence stars in the Galactic globular cluster 47 Tucanae (NGC 104).
A. A. Zijlstra +62 more
core +1 more source

