Results 61 to 70 of about 462 (193)
An Enhanced Hertzsprung–Russell Diagram Using Gaia EDR3 Data
Wei‐Chun Jao, Gregory A. Feiden
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An AGN Hertzsprung-Russell Diagram
Contribution for Elba Conference "Issues in Unification of AGNs"
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Theoretical interpretation of the Hertzsprung-Russell diagram [PDF]
The theory of the stellar interior indicates that for a star of given mass, given initial composition, and given age, all physical characteristics (including the luminosity and the effective temperature) are uniquely determined. Accordingly it should be possible to derive theoretically for a particular star of definite mass and initial composition a ...
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Stellar X-Ray Activity Across the Hertzsprung–Russell Diagram. I. Catalogs [PDF]
Song Wang, Yu Bai, Lin He, Jifeng Liu
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A Comprehensive Study of Czernik 41 and NGC 1342 Using CCD UBV and Gaia DR3 Data
In this study, the structural, astrophysical, kinematic, and Galactic orbital parameters of the open clusters Czernik 41 and NGC 1342, as well as their dynamical evolution, are investigated using CCD UBV photometry and Gaia data.
Burçin Tanık Öztürk +7 more
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Evaluating Gaia Astrometric Quality and Distances for Galactic Hot Supergiants
Distances to Galactic BA supergiants are essential for determining their luminosities, radii, and positions on the Hertzsprung–Russell diagram, yet Gaia parallaxes for these bright, extended sources are often affected by systematics.
Nadezhda L. Vaidman +5 more
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The HIPPARCOS Hertzsprung-Russell diagram of S stars: Probing\n nucleosynthesis and dredge-up [PDF]
S. Van Eck +4 more
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Hα Emission among Evolved FGKM Stars: A Compendium from the Literature
Emission in the wings of the H α line among late-type giant stars occurs as a consequence of conditions in their chromospheres. Data from the literature have been used to document the incidence of H α emission among Population I giant stars as a function
Graeme H. Smith
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The Internal Kinematics of NGC 2808 and Its Multiple Populations
We use new Hubble Space Telescope observations coupled with archival data spanning a total temporal baseline of 17 yr to study the internal kinematics of the multiple populations in the globular cluster NGC 2808 from its center out to ∼8 half-light radii
M. Griggio +12 more
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The imprint of star formation on stellar pulsations. [PDF]
Steindl T, Zwintz K, Vorobyov E.
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