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  2. WR 102 - Wikipedia

    en.wikipedia.org/wiki/WR_102

    WR 102 was first mentioned as the possible optical counterpart to a peculiar X-ray source GX 3+1. [6] However, it became clear that it was a separate object and in 1971 it was highlighted as a luminous star with unusual O VI emission lines in its spectrum. [7]

  3. WR 102c - Wikipedia

    en.wikipedia.org/wiki/WR_102c

    WR 102c is surrounded by a shell of nebulosity which contains dust made even hotter than the star itself by intense radiation. The nebula also includes nearly 1 M ☉ of molecular hydrogen and around 10 M ☉ of ionised hydrogen, all expelled from the star. [4] There is a suggestion that WR 102c may be a binary star.

  4. WR 102ea - Wikipedia

    en.wikipedia.org/wiki/WR_102ea

    WR 102ea is a Wolf–Rayet star in the Sagittarius constellation. It is the third most luminous star in the Quintuplet cluster after WR 102hb . With a luminosity of 2,500,000 times solar , it is also one of the most luminous stars known.

  5. WR 102ka - Wikipedia

    en.wikipedia.org/wiki/WR_102ka

    Narrowband infrared observations of several spectral features around 2 μm showed that WR 102ka was a Wolf Rayet star with a likely classification of WN10. [7] It was also proposed as a possible luminous blue variable. [8] The Spitzer Space Telescope observed WR 102ka at wavelengths of 3.6 μm, 8 μm, and 24 μm on April 20, 2005. These ...

  6. List of Wolf-Rayet stars - Wikipedia

    en.wikipedia.org/wiki/List_of_Wolf-Rayet_stars

    This is a list of Wolf-Rayet stars, in order of their distance from Earth. [1] [2] [3] List ... WR 102: 9,500 ± 600: 1: WO2: 14.10: WR 138: 10,000: 1: WR: WR 1: ...

  7. Wolf–Rayet star - Wikipedia

    en.wikipedia.org/wiki/Wolf–Rayet_star

    WR 136, a WN6 star where the atmosphere shed during the red supergiant phase has been shocked by the hot, fast WR winds to form a visible bubble nebula. In 1867, using the 40 cm Foucault telescope at the Paris Observatory, astronomers Charles Wolf and Georges Rayet [1] discovered three stars in the constellation Cygnus (HD 191765, HD 192103 and HD 192641, now designated as WR 134, WR 135, and ...

  8. List of supernova candidates - Wikipedia

    en.wikipedia.org/wiki/List_of_supernova_candidates

    The list includes massive Wolf–Rayet stars, which may become Type Ib/Ic supernovae, particularly oxygen-sequence (Wolf-Rayet WO) stars. As of 2023, most of these candidates are in the Milky Way galaxy, however five oxygen-sequence Wolf-Rayet stars are also known in other galaxies.

  9. Orders of magnitude (power) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(power)

    astro: luminosity per square meter of the hottest normal star known, WR 102: 5–20 × 10 13: weather: rate of heat energy release by a hurricane [citation needed] 10 14: 1.4 × 10 14: eco: global net primary production (= biomass production) via photosynthesis [47] 2.9 × 10 14

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