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We consider a (very) simple version of the restricted three body problem in general relativity. The background geometry is given by a Schwarzschild solution governing the motion of two bodies of masses $$m_1$$ and $$m_2$$. We assume that corrections to the trajectory of the body of mass $$m_1$$ due to the presence of the mass $$m_2$$ are given by a Newtonian approximation where Poisson's equation is solved with respect to the Schwarzschild background geometry. Under these assumptions, we derive approximate equations of motion for the corrections to the trajectory of the body of mass $$m_1$$.
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A shock flash breaking out of a dusty red supergiant
This record contains the data of spectra and photometry used for the paper A shock flash breaking out of a dusty red supergiant [MJD]_[Band]_[Instrument]_[stacked number x exposure time of a single image].fits - Images of SN2023ixf after reduction code.zip - Code to fit the hybrid model
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- Award ID(s):
- 1817099
- PAR ID:
- 10569369
- Publisher / Repository:
- Zenodo
- Date Published:
- Format(s):
- Medium: X
- Right(s):
- Closed Access
- Sponsoring Org:
- National Science Foundation
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