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R Serpentis

Variable star in the constellation Serpens

Summary

Variable star in the constellation Serpens

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R Serpentis is a Mira variable type star in the equatorial constellation of Serpens. It ranges between apparent magnitude 5.16 and 14.4, and spectral types M5e to M8e, over a period of 356.41 days. When it is near maximum brightness, it can be seen with the naked eye under excellent observing conditions. The variability of this star was discovered in 1826 by Karl Ludwig Harding.

References

| display-authors=1 | last1=Keenan | first1=Philip C.

References

  1. "Download Data". AAVSO.
  2. "R Ser".
  3. {{cite DR2
  4. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society.
  5. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost". Astronomy and Astrophysics.
  6. (2016). "Pulsation-triggered Mass Loss from AGB Stars: The 60 Day Critical Period". The Astrophysical Journal.
  7. (1994). "Three Early Variable Star Catalogues". Journal for the History of Astronomy.
Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

m-type-giants mira-variables serpens durchmusterung-objects henry-draper-catalogue-objects hipparcos-objects bright-star-catalogue-objects objects-with-variable-star-designations
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