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The Early Years in White Dwarf Research - Gravitational Red Shifts?

Автор: Sky Scholar

Загружено: 2024-02-02

Просмотров: 6308

Описание:

J.B. Holberg, Sirius Brightest Diamond in the Night Sky, Springer, New York, 2007.

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D. Saumon, S. Blouin, and P.E. Tremblay, Current challenges in the physics of white dwarf stars, Physics Reports, 2022, 988, 1-63.

V. Chandra, H.-C. Hwang, N.L. Zakamska, and S. Cheng, A gravitational redshift measurement of the white dwarf mass-radius relation, Astrophys. J. 2020, 999, 146 (9pp)

L.K. Rogers et al., WE0141-675: A case study on how to follow-up astrometric candidates around white dwarfs, Mon. Not. Roy. Astron. Soc. 2024, 527, 977-990.

A.S. Adams, The relativity displacement of the spectral lines in the companion of Sirius, Proc. Nat. Acad. Sci. 1925, 11, 382-387.

J.H. Moore, Recent spectrographic observations of the companion of Sirius, Pub. Astron. Soc. Pac. 1928, 40, 229-233.

D.M. Popper, Red shift in the spectrum of 40 Eridani B, Astrophys. J. 1954, 120, 316-321.

J.L. Greenstein and V. Trimble, The gravitational redshift of 40 Eridani B, Astrophys. J. 1972, 175, L1-L5.

J.L. Greenstein, and V.L. Trimble, The Einstein Redshift in White Dwarfs, Astrophys. J. 1967, 149, 283-298.

P. Chayer, G. Fontaine, and F Wesemael, Radiative Levitation in Hot White Dwarfs: Equilibrium Theory, Astrophys. J. Suppl. Ser. 1995, 99, 189-221.

P. Chayer and, J. Dupuis, Effect of Radiative Levitation on Calculations of Accretion Rates in White Dwarfs, AIP Conf. Proc. 2010, 1273, 394–399.

D. Aumiler, T. Ban, and G. Pichler, High-resolution measurements of the pressure broadening and shift of the rubidium 52S1∕2–62P3∕2 line by argon and helium, Phys. Rev. A 2004, 70, 032723 – Published 30 September 2004

M.A. Bouchiat, J. Brossel, P. Mora, and L. Pottier, Properties of rubidium-argon Van der Waals molecules from the relaxation of polarized Rb atoms, J. Phys. France 1975, 36, 1075-1077.

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A.S. Eddington, The internal constitution of the stars, Cambridge University Press, 1926, p. 170-174.

The Life Cycle of the Stars | Pierre-Marie Robitaille [OTF2017]
   • The Life Cycle of the Stars | Pierre-Marie...  

The Main Sequence of the Stars: What is the Most Likely Structure?
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EXTREME Density! The White Dwarf Star, Eddington, and Thermodynamics!
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Thank you for viewing this video on Sky Scholar! This channel is dedicated to new ideas about the nature of the sun, the stars, thermodynamics, and the microwave background. We will discuss all things astronomy, physics, chemistry, and imaging related! We hope that the combination of facts and special effects will aid in learning even the toughest concepts in astronomy. If you enjoyed this video, please subscribe.

Pierre-Marie Robitaille, Ph.D., was a professor of Radiology at The Ohio State University from 1989-2019, and also held an appointment in the Chemical Physics Program. In 1998, he led the design and assembly of the world’s first Ultra High Field MRI System. Readings from this equipment brought into question fundamental aspects of modern thermal physics, such as Kirchhoff’s Law of thermal emission.

Outro Music:
Foria: Break Away

  / foria  
   • Foria - Break Away | Melodic Dubstep | NCS...  

The Early Years in White Dwarf Research - Gravitational Red Shifts?

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