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  1. P Cygni - Wikipedia

    • P Cygni (34 Cygni) is a variable star in the constellation Cygnus. The designation "P" was originally assigned by Johann Bayer in Uranometria as a nova. Located in about 5,300 light-years (1,560 parsecs) from Earth, it is a hypergiant luminous blue variable (LBV) star of spectral type B1-2 Ia-0ep that is one of the most luminous stars in the Milky Way. … See more

    Visibility

    The star is located about 5,000 to 6,000 light-years (1,500–1,800 parsecs) from Earth. Despite this vast distance, it is visible … See more

    Luminous blue variable P Cygni

    P Cygni is widely considered to be the earliest known example of a luminous blue variable. However, it is far from a typical example. Typically, LBVs change in brightness with a period of years to decades, o… See more

    ConstellationCygnus
    Right ascension20ʰ 17ᵐ 47.2020ˢ
    Declination+38° 01′ 58.549″
    Apparent magnitude (V)4.82 (3 to 6)
    Evolution

    Luminous blue variables like P Cygni are very rare and short lived, and only form in regions of galaxies where intense star formation is happening. LBV stars are so massive and energetic (typically 50 times the mass o… See more

    P Cygni profile

    P Cygni gives its name to a type of spectroscopic feature called a P Cygni profile, where the presence of both absorption and emission in the profile of the same spectral line indicates the existence of a gaseous … See more

    Companion

    It has been proposed P Cygni's eruptions could be caused by mass transfer to a hypothetical companion star of spectral type B that would have a mass between 3 and 6 times the mass of the Sun and would orbit P Cygni ea… See more

     
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  2. P Cygni - Astronomy Magazine

    Jan 1, 2024 · Seen through binoculars and backyard telescopes, P Cygni is an unassuming sight, a speck of sapphire starlight. What’s invisible to our eyes are the shells of dust and gas that P Cygni...

     
  3. P Cygni Star Facts - Universe Guide

  4. P Cygni - aavso

    The September 2009 Variable Star of the Season is P Cygni, one of the rare S Doradus or luminous blue variable stars, and the namesake for a curious phenomenon in astrophysics. Read on for more about this bright but …

  5. P Cyg - University of Illinois Urbana-Champaign

  6. P Cygni stars - Astrosurf

  7. Identification of Spectral Lines - History of P-Cygni lines

    These 'P-Cygni' lines are a characteristic common to all novae and stars with strong mass ejections or violent stellar winds such as Eta Carinae. The stellar 'ashes' that accumulate often take the form of a circumstellar nebula of gas …

  8. P Cygni profile - David Darling

  9. P Cygni - Conservapedia

  10. P Cygni - Simple English Wikipedia, the free encyclopedia

  11. P-Cygni Profile (Robert Eder) - AstroBin

    The P-Cygni profile of a spectral line is created by a stellar wind and is characterized by a broad, unshifted emission line, which is bounded on the blue side by a narrow, blue-shifted absorption line (marked in the yellow circle).

  12. P Cygni: An Extraordinary Luminous Blue Variable - ADS

  13. Title: P Cygni: An Extraordinary Luminous Blue Variable - arXiv.org

  14. The H-alpha Variations of the Luminous Blue Variable P Cygni: …

  15. P Cygni: An Extraordinary Luminous Blue Variable

  16. P-Cygni Animations - Lawrence Berkeley National Laboratory

  17. The P Cygni Profile and Friends - SpringerLink

  18. Characteristics of the Variable Star P Cygni Determined from …

  19. P Cygni: The Star that Started it All | SpringerLink

  20. 61 Cygni - Wikipedia

  21. Understanding the P Cygni Profile - SpringerLink