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

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Reference Type	Journal (article/letter/editorial)
Title	Possible Overionization of C II, N II, and O II Ions in the Atmospheres of Early B- and Late O-Type Stars
Journal	Astrophysics
Authors	Lyubimkov, L. S.		Author
Year	2013 (December)	Volume	56
Issue	4
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/s10511-013-9301-xSearch in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3596366	Long-form Identifier	mindat:1:5:3596366:2
GUID	0
Full Reference	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
Plain Text	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
In	(2013, December) Astrophysics Vol. 56 (4) Springer Science and Business Media LLC

	*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*
	*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*
	*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*
	Colucci, G., Mannarelli, M., Manuel, C. (2013) r-Mode Oscillations and Rocket Effect in Rotating Superfluid Neutron Stars. II. Numerical Results. Astrophysics, 56 (1). 104-120 doi:10.1007/s10511-013-9271-z
	*Petrosyan, G. V. (2013) Classification of KP2001 stars using spectra obtained with a slit spectrograph. II. Astrophysics, 56 (3). 421-430 doi:10.1007/s10511-013-9296-3*
	*Lyubimkov, L. S. (1984) Evolutionary increase in the nitrogen abundance in the atmospheres of early B stars. Astrophysics, 20 (3). 255-266 doi:10.1007/bf01005414*
	*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*
	*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*
	Rojas, M., Drake, N. A., Chavero, C., Pereira, C. B., Kholtygin, A. F., Solovyov, D. I. (2013) Analysis of the Chemical Composition of the Atmospheres of Stars with Debris Disks and Planetary Systems. Astrophysics, 56 (4). 461-471 doi:10.1007/s10511-013-9300-y
	*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. (1977) Variations in the helium abundance in associations and clusters of O and B stars. Astrophysics, 13 (1). 71-78 doi:10.1007/bf01003156*

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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

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