Introducing a new multi-particle collision method for the evolution of dense stellar systems. II. Core collapse

Introducing a new multi-particle collision method for the evolution of dense stellar systems. Crash-test N-body simulations

Astronomy and Astrophysics ◽

10.1051/0004-6361/202038784 ◽

2021 ◽

Author(s):

P. Di Cintio ◽

M. Pasquato ◽

H. Kim ◽

S.-J. Yoon

Keyword(s):

Particle Collision ◽

Crash Test ◽

Stellar Systems

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Homologous evolution of stellar systems after core collapse

The Astrophysical Journal ◽

10.1086/161996 ◽

1984 ◽

Vol 280 ◽

pp. 298 ◽

Cited By ~ 58

Author(s):

J. Goodman

Keyword(s):

Stellar Systems ◽

Core Collapse

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Desiderata in connection by the calibration of the MK-system

Symposium - International Astronomical Union ◽

10.1017/s0074180900053699 ◽

1966 ◽

Vol 24 ◽

pp. 348-349

Author(s):

Th. Schmidt-Kaler

Keyword(s):

Absolute Magnitude ◽

Review Article ◽

Stellar Systems ◽

Astronomical Data ◽

Intrinsic Colour

This is only an informal remark about some difficulties I am worrying about.I have tried to recalibrate the MK system in terms of intrinsic colour (B–V)0and absolute magnitudeMv. The procedures used have been described in a review article by Voigt (Mitt. Astr. Ges.1963, p. 25–35), and the results for stars of the luminosity classes Ia-O,I and II have been given also in Blaauw's article on the calibration of luminosity criteria in vol. III (Basic Astronomical Data, p. 401) ofStars and Stellar Systems.

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Symbiotic Stars at Optical, Infrared and Radio Wavelengths

International Astronomical Union Colloquium ◽

10.1017/s025292110007336x ◽

1979 ◽

Vol 46 ◽

pp. 125-149 ◽

Cited By ~ 3

Author(s):

David A. Allen

Keyword(s):

Temperature Regime ◽

Type Star ◽

Stellar Systems ◽

Symbiotic Stars ◽

Lower Excitation ◽

Definition Of ◽

Original Type

No paper of this nature should begin without a definition of symbiotic stars. It was Paul Merrill who, borrowing on his botanical background, coined the termsymbioticto describe apparently single stellar systems which combine the TiO absorption of M giants (temperature regime ≲ 3500 K) with He II emission (temperature regime ≳ 100,000 K). He and Milton Humason had in 1932 first drawn attention to three such stars: AX Per, CI Cyg and RW Hya. At the conclusion of the Mount Wilson Ha emission survey nearly a dozen had been identified, and Z And had become their type star. The numbers slowly grew, as much because the definition widened to include lower-excitation specimens as because new examples of the original type were found. In 1970 Wackerling listed 30; this was the last compendium of symbiotic stars published.

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