Results 301 to 310 of about 299,299 (345)
Ultrasound-Guided Synovial Biopsy in Undifferentiated Monoarthritis: A Case Series From Bangladesh. [PDF]
CureusAzad MAK +4 more
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Nanoengineering of Lu(III) Bisphthalocyanine-Cored Polycaprolactone Polymers and Nanoparticles. [PDF]
ACS OmegaEmami A +7 more
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Thoracoscopic Resection of a Giant Solitary Fibrous Tumor in the Chest Cavity After Preoperative Arterial Embolization: A Case Report. [PDF]
CureusTakada I +10 more
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Prospects for detecting signs of life on exoplanets in the JWST era. [PDF]
Proc Natl Acad Sci U S ASeager S +4 more
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Journal of Astrophysics and Astronomy, 1989
This study is part of an investigation of the possibility of using chemically peculiar (CP) stars to map local galactic structure. Correct luminosities of these stars are therefore crucial. CP stars are generally regarded as main-sequence or near-main-sequence objects. However, some CP stars have been classified as giants.
L. O. Lodén, A. Sundman
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This study is part of an investigation of the possibility of using chemically peculiar (CP) stars to map local galactic structure. Correct luminosities of these stars are therefore crucial. CP stars are generally regarded as main-sequence or near-main-sequence objects. However, some CP stars have been classified as giants.
L. O. Lodén, A. Sundman
openaire +1 more source
2008
Long-period radial velocity (RV) variations were discovered over 13 years ago in the K giant stars β Gem, α Tau, and α Boo by [1]. One hypothesis for these variations was that they were caused by substellar companions with masses of 2–11 M Jupiter and orbital semi-major axes of ≈ 2 AU.
A. P. Hatzes +5 more
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Long-period radial velocity (RV) variations were discovered over 13 years ago in the K giant stars β Gem, α Tau, and α Boo by [1]. One hypothesis for these variations was that they were caused by substellar companions with masses of 2–11 M Jupiter and orbital semi-major axes of ≈ 2 AU.
A. P. Hatzes +5 more
openaire +1 more source
EAS Publications Series, 2006
The observed brightness fluctuations and large-scale structures on the surface of the Red Supergiant Betelgeuse make the star a prime targed for future interferometric measurements. At the same time, they open the possibility to resolve these structures in numerical radiation hydrodynamics simulations of the entire star.
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The observed brightness fluctuations and large-scale structures on the surface of the Red Supergiant Betelgeuse make the star a prime targed for future interferometric measurements. At the same time, they open the possibility to resolve these structures in numerical radiation hydrodynamics simulations of the entire star.
openaire +1 more source