Bell, G. D., Paquette, D. R., Wiese, W. L. (1966) Relative Transition Probabilities for Prominent NI i and NI II Lines in the Near-Ultraviolet. The Astrophysical Journal, 143. 559pp. doi:10.1086/148534

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Reference Type	Journal (article/letter/editorial)
Title	Relative Transition Probabilities for Prominent NI i and NI II Lines in the Near-Ultraviolet
Journal	The Astrophysical Journal
Authors	Bell, G. D.		Author
	Paquette, D. R.		Author
	Wiese, W. L.		Author
Year	1966 (February)	Volume	143
Publisher	IOP Publishing
DOI	doi:10.1086/148534Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3301756	Long-form Identifier	mindat:1:5:3301756:1
GUID	0
Full Reference	Bell, G. D., Paquette, D. R., Wiese, W. L. (1966) Relative Transition Probabilities for Prominent NI i and NI II Lines in the Near-Ultraviolet. The Astrophysical Journal, 143. 559pp. doi:10.1086/148534
Plain Text	Bell, G. D., Paquette, D. R., Wiese, W. L. (1966) Relative Transition Probabilities for Prominent NI i and NI II Lines in the Near-Ultraviolet. The Astrophysical Journal, 143. 559pp. doi:10.1086/148534
In	(1966) The Astrophysical Journal Vol. 143. IOP Publishing

	Bell, G. D., Paquette, D. R., Wiese, W. L. (1966) Relative Transition Probabilities for Prominent NI I and NI II Lines in the Near Ultraviolet. The Astronomical Journal, 71. 156pp. doi:10.1086/110001
	Nitz, D. E., Kunau, A. E., Wilson, K. L., Lentz, L. R. (1999) Atomic Transition Probabilities for Visible and Near‐Ultraviolet Spectral Lines in Co i. The Astrophysical Journal Supplement Series, 122 (2) 557-561 doi:10.1086/313223
	*Mendlowitz, H. (1966) Calculated Line Strengths for the Transition Array for d^{2}s-d^{2}p: Application to NI II. The Astrophysical Journal, 143. 573pp. doi:10.1086/148535*
	*Bridges, J. M., Wiese, W. L. (1970) Transition Probabilities for the Prominent Red Lines of Ne I. Physical Review A, 2 (2). 285-293 doi:10.1103/physreva.2.285*
	*Calamai, Anthony G., Smith, Peter L., Bergeson, S. D. (1993) Transition probabilities for the 3s2 3p(2P0)-3s3p2(4P) intersystem lines of SI II. The Astrophysical Journal, 415. doi:10.1086/187032*
	*Lennard, W. N., Whaling, W., Scalo, J. M., Testerman, L. (1975) NI I transition probabilities and the solar nickel abundance. The Astrophysical Journal, 197. 517pp. doi:10.1086/153538*
	*King, Robert B. (1948) Relative gƒ-VALUES for Lines of NI I. The Astrophysical Journal, 108. 87pp. doi:10.1086/145045*
	*Veres, G., Wiese, W. L. (1996) Experimental atomic transition probabilities for O II lines. Physical Review A, 54 (3). 1999-2003 doi:10.1103/physreva.54.1999*
	Berg, H. F., Eckerle, K. L., Burris, R. W., Wiese, W. L. (1964) Relative Oscillator Strengths of Some O II and O III Lines from Measurements on Shock-Heated Plasmas. The Astrophysical Journal, 139. 751pp. doi:10.1086/147800
	*Quinet, P., Le Dourneuf, M. (1996) Transition probabilities for [Ni I] and [Ni II] lines. Astronomy and Astrophysics Supplement Series, 119. 99-104 doi:10.1051/aas:1996230*
	*Miller, Myron H., Bengtson, Roger D. (1969) Relative Transition Probabilities for Silicon. The Astrophysical Journal, 156. 393pp. doi:10.1086/149976*

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Bell, G. D., Paquette, D. R., Wiese, W. L. (1966) Relative Transition Probabilities for Prominent NI i and NI II Lines in the Near-Ultraviolet. The Astrophysical Journal, 143. 559pp. doi:10.1086/148534

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