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

Zinātniskās darbības rezultāts: Nodaļa grāmatā/enciklopēdijā/konferences krājumā › Konferences zinātniskais raksts › Pētniecība › koleģiāli recenzēts

Oriģinālvaloda	Angļu
Rīkotāja publikācijas nosaukums	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.
Publikācijas vieta	Cambridge
Izdevējs	Cambridge University Press
Lapas	167-170
DOIs	https://doi.org/10.1017/S1743921310000475
Publikācijas statuss	Publicēts - 2010

Publikāciju sērijas

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

OECD Zinātnes nozare

1.3 Fizika un astronomija

Piekļuve Dokumentiem

10.1017/S1743921310000475

Citēt šo

Docenko, D. (2010). Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. (gadā) 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. (lpp. 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. lpp. 167-170 (IAU Symposium Proceedings Series ; Vol.5, N 265).

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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. (kur) 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, lpp. 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. lpp. 167-170 (IAU Symposium Proceedings Series ; Vol.5, N 265).

Zinātniskās darbības rezultāts: Nodaļa grāmatā/enciklopēdijā/konferences krājumā › Konferences zinātniskais raksts › Pētniecība › koleģiāli recenzēts

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AU - Docenko, Dmitrijs

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DO - 10.1017/S1743921310000475

M3 - Conference paper

T3 - IAU Symposium Proceedings Series ; Vol.5, N 265

SP - 167

EP - 170

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.

PB - Cambridge University Press

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Docenko D. Possibility of measuring the amount of intergalactic metals with N-14 VII HFS line. (gadā) 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. lpp. 167-170. (IAU Symposium Proceedings Series ; Vol.5, N 265). doi: 10.1017/S1743921310000475