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Reference Type	Journal (article/letter/editorial)
Title	The N/O Ratio in Early B-Type Main Sequence Stars as an Indicator of Their Evolution
Journal	Astrophysics
Authors	Lyubimkov, L. S.		Author
Year	2016 (December)	Volume	59
Issue	4
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/s10511-016-9449-2Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3596527	Long-form Identifier	mindat:1:5:3596527:1
GUID	0
Full Reference	Lyubimkov, L. S. (2016) The N/O Ratio in Early B-Type Main Sequence Stars as an Indicator of Their Evolution. Astrophysics, 59 (4). 461-474 doi:10.1007/s10511-016-9449-2
Plain Text	Lyubimkov, L. S. (2016) The N/O Ratio in Early B-Type Main Sequence Stars as an Indicator of Their Evolution. Astrophysics, 59 (4). 461-474 doi:10.1007/s10511-016-9449-2
In	(2016, December) Astrophysics Vol. 59 (4) Springer Science and Business Media LLC

	*Lyubimkov, L. S. (2013) Possible Overionization of C II, N II, and O II Ions in the Atmospheres of Early B- and Late O-Type Stars. Astrophysics, 56 (4). 472-487 doi:10.1007/s10511-013-9301-x*
	*Lyubimkov, L. S. (2016) Lithium in Stellar Atmospheres: Observations and Theory. Astrophysics, 59 (3). 411-437 doi:10.1007/s10511-016-9446-5*
	*Lyubimkov, L. S. (1996) Observational manifestations of early mixing in B- and O-type stars. Astrophysics and Space Science, 243 (2). 329-349 doi:10.1007/bf00644704*
	*Lyubimkov, L. S. (2018) Light Chemical Elements in Stars: Mysteries and Unsolved Problems. Astrophysics, 61 (2). 262-285 doi:10.1007/s10511-018-9533-x*
	*Melikian, N. D., Karapetian, A. A., Gomez, J. (2016) New Emission Stars in B Cyg OB7. Astrophysics, 59 (4). 484-491 doi:10.1007/s10511-016-9451-8*
	*Glagolevskij, Yu. V. (2013) Evolution of the magnetic fields of main-sequence CP-stars. II. Astrophysics, 56 (3). 407-420 doi:10.1007/s10511-013-9295-4*
	*Lyubimkov, L. S. (1989) Correlation between the helium abundances in the atmospheres of early B stars and their ages and masses. Astrophysics, 29 (3). 704-713 doi:10.1007/bf01004212*
	*Glagolevskij, Yu. V. (2013) Evolution of the magnetic fields of main-sequence CP-stars. I. Astrophysics, 56 (2). 173-190 doi:10.1007/s10511-013-9277-6*
	*Glagolevskij, Yu. V. (2014) Evolution of the Magnetic Fields of Main-Sequence CP-Stars. III. Astrophysics, 57 (2). 204-212 doi:10.1007/s10511-014-9326-9*
	*Morchenko, E. S. (2016) Origin of the Blue Continuum Radiation in the Flare Spectra of dMe Stars. Astrophysics, 59 (4). 475-483 doi:10.1007/s10511-016-9450-9*
	*Glagolevskij, Yu. V. (2016) Magnetic Stars After the Hayashi Phase. I. Astrophysics, 59 (2). 164-182 doi:10.1007/s10511-016-9425-x*

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Lyubimkov, L. S. (2016) The N/O Ratio in Early B-Type Main Sequence Stars as an Indicator of Their Evolution. Astrophysics, 59 (4). 461-474 doi:10.1007/s10511-016-9449-2

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