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Aggarwal, K. M., Keenan, F. P. (2003) Excitation rates for transitions in Ca XV. Astronomy & Astrophysics, 407 (2). 769-778 doi:10.1051/0004-6361:20030874

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Reference TypeJournal (article/letter/editorial)
TitleExcitation rates for transitions in Ca XV
JournalAstronomy & Astrophysics
AuthorsAggarwal, K. M.Author
Keenan, F. P.Author
Year2003 (August)Volume407
Issue2
PublisherEDP Sciences
DOIdoi:10.1051/0004-6361:20030874Search in ResearchGate
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Mindat Ref. ID3461323Long-form Identifiermindat:1:5:3461323:8
GUID0
Full ReferenceAggarwal, K. M., Keenan, F. P. (2003) Excitation rates for transitions in Ca XV. Astronomy & Astrophysics, 407 (2). 769-778 doi:10.1051/0004-6361:20030874
Plain TextAggarwal, K. M., Keenan, F. P. (2003) Excitation rates for transitions in Ca XV. Astronomy & Astrophysics, 407 (2). 769-778 doi:10.1051/0004-6361:20030874
In(2003, August) Astronomy & Astrophysics Vol. 407 (2) EDP Sciences

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Aggarwal, K. M., Keenan, F. P. (2007) Energy levels, radiative rates and excitation rates for transitions in Ni XI. Astronomy & Astrophysics, 475 (1). 393-399 doi:10.1051/0004-6361:20078561
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Aggarwal, K. M., Keenan, F. P. (2008) Energy levels, radiative rates, and electron impact excitation rates for transitions in O VII. Astronomy & Astrophysics, 489 (3). 1377-1388 doi:10.1051/0004-6361:200810531
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Aggarwal, K. M., Kato, T., Keenan, F. P., Murakami, I. (2009) Radiative rates and electron impact excitation rates for transitions in Cr VIII. Astronomy & Astrophysics, 506 (3). 1501-1509 doi:10.1051/0004-6361/200912493
Aggarwal, K. M., Keenan, F. P. (2003) Effective collision strengths for transitions in Fe XI. Astronomy & Astrophysics, 399 (2). 799-805 doi:10.1051/0004-6361:20021733
Aggarwal, K. M., Keenan, F. P., Nakazaki, S. (2005) Energy levels and radiative rates for transitions in Ar XIII, Ar XIV and Ar XV. Astronomy & Astrophysics, 436 (3). 1141-1150 doi:10.1051/0004-6361:20052847
Aggarwal, K. M., Keenan, F. P. (2004) Radiative rates for E1, E2, M1 and M2 transitions in Fe X. Astronomy & Astrophysics, 427 (2). 763-767 doi:10.1051/0004-6361:20040300
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