On the period of VY Ursae Majoris

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This article contains visual observation data of the carbon star VY Ursae Majoris.

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2 p.

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Ofek, Efran; Shemmer, Ohad & Gabzo, Ofer May 25, 1994.

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  • © 1994 The Authors

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Description

This article contains visual observation data of the carbon star VY Ursae Majoris.

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2 p.

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Abstract: The carbon star VY Ursae Majoris is catalogued as an Lb irregular variable. Visual observations indicate that the star is more likely to be a semi-regular variable. Visual observations made in 1990-1993 reveal a clear period of 120 days for the star, with probably long-term changes in mean brightness.

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  • Journal of British Astronomical Association, 1995. London, UK: British Astronomical Association

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  • Publication Title: Journal of British Astronomical Association
  • Volume: 105
  • Issue: 1
  • Page Start: 33
  • Page End: 34

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  • May 25, 1994

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  • Aug. 8, 2018, 8:27 a.m.

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Ofek, Efran; Shemmer, Ohad & Gabzo, Ofer. On the period of VY Ursae Majoris, article, May 25, 1994; London, United Kingdom. (digital.library.unt.edu/ark:/67531/metadc1225769/: accessed November 19, 2018), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT College of Arts and Sciences.