Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line

Dmitrijs Docenko

doi:10.1017/S1743921310000475

Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line

Dmitrijs Docenko

Research output: Chapter in Book/Report/Conference proceeding › Conference paper › Research › peer-review

Original language	English
Title of host publication	Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009.
Place of Publication	Cambridge
Publisher	Cambridge University Press
Pages	167-170
DOIs	https://doi.org/10.1017/S1743921310000475
Publication status	Published - 2010

Publication series

Name	IAU Symposium Proceedings Series ; Vol.5, N 265

OECD Field of Science

1.3 Physical Sciences

Access to Document

10.1017/S1743921310000475

Cite this

Docenko, D. (2010). Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. In Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009. (pp. 167-170). (IAU Symposium Proceedings Series ; Vol.5, N 265). Cambridge University Press. https://doi.org/10.1017/S1743921310000475

Docenko, Dmitrijs. / Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009.. Cambridge : Cambridge University Press, 2010. pp. 167-170 (IAU Symposium Proceedings Series ; Vol.5, N 265).

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title = "Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line",

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language = "English",

series = "IAU Symposium Proceedings Series ; Vol.5, N 265",

publisher = "Cambridge University Press",

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Docenko, D 2010, Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. in Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009.. IAU Symposium Proceedings Series ; Vol.5, N 265, Cambridge University Press, Cambridge, pp. 167-170. https://doi.org/10.1017/S1743921310000475

Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. / Docenko, Dmitrijs.
Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009.. Cambridge: Cambridge University Press, 2010. p. 167-170 (IAU Symposium Proceedings Series ; Vol.5, N 265).

Research output: Chapter in Book/Report/Conference proceeding › Conference paper › Research › peer-review

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BT - Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009.

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Docenko D. Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. In Chemical abundances in the Universe: connecting first stars to planets: proceedings of the 265th symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009.. Cambridge: Cambridge University Press. 2010. p. 167-170. (IAU Symposium Proceedings Series ; Vol.5, N 265). doi: 10.1017/S1743921310000475