天龍座BY型變星 (Chinese Wikipedia)
Analysis of information sources in references of the Wikipedia article "天龍座BY型變星" in Chinese language version.
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arxiv.org
- Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S., Limits to Transits of the Neptune-mass planet orbiting Gl 581, Publications of the Astronomical Society of the Pacific, 2006, 118 (849): 1506, Bibcode:2006PASP..118.1506L, arXiv:astro-ph/0609255
, doi:10.1086/508904, BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.
books.google.com
- Schrijver, Carolus J.; Zwaan, Cornelis, Solar and stellar magnetic activity, Cambridge astrophysics series 34, Cambridge University Press: 343, 2000 [2018-06-20], ISBN 0-521-58286-5, （原始内容存档于2021-02-14）
- Jaschek, Carlos; Jaschek, Mercedes, The Classification of Stars, Cambridge University Press: 374, 1990 [2018-06-20], ISBN 0-521-38996-8, （原始内容存档于2021-02-14）
doi.org
- Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S., Limits to Transits of the Neptune-mass planet orbiting Gl 581, Publications of the Astronomical Society of the Pacific, 2006, 118 (849): 1506, Bibcode:2006PASP..118.1506L, arXiv:astro-ph/0609255 , doi:10.1086/508904,
BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.
harvard.edu
ui.adsabs.harvard.edu
- Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S., Limits to Transits of the Neptune-mass planet orbiting Gl 581, Publications of the Astronomical Society of the Pacific, 2006, 118 (849): 1506, Bibcode:2006PASP..118.1506L, arXiv:astro-ph/0609255 , doi:10.1086/508904,
BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.
web.archive.org
- Schrijver, Carolus J.; Zwaan, Cornelis, Solar and stellar magnetic activity, Cambridge astrophysics series 34, Cambridge University Press: 343, 2000 [2018-06-20], ISBN 0-521-58286-5, （原始内容存档于2021-02-14）
- Jaschek, Carlos; Jaschek, Mercedes, The Classification of Stars, Cambridge University Press: 374, 1990 [2018-06-20], ISBN 0-521-38996-8, （原始内容存档于2021-02-14）