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A quest for weak objects and for invisible stars

1998/01/04 by С. И. Блинников, S. I. Blinnikov, Blinnikov, S. I. · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9801015

6 pages LaTeX, presented at "Baryonic Matter in the Universe and Its Spectroscopic Studies" (November 22 - 24, 1996, Atami, Japan)

arxiv created 1998/01/04 · openalex publication_date 1998/01/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

High quality spectra to be produced by SUBARU 8 meter telescope will be extremely valuable for numerous astronomical projects. Here I concentrate on two classical types of weak broad line objects -- distant supernovae and white dwarfs -- with emphasis of their importance for fundamental physics, not only for astronomy. With regard to recent results of MACHO experiment and HST weak star counts I discuss one exotic possibility: invisible stars made of the so called ``mirror'' matter.

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