Standard

From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe. / Voshchinnikov, N.V.; Henning, Th.

в: ASTRONOMY & ASTROPHYSICS, Том 517, 2010, стр. A45.

Результаты исследований: Научные публикации в периодических изданиях › статья

Harvard

Voshchinnikov, NV & Henning, T 2010, 'From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe', ASTRONOMY & ASTROPHYSICS, Том. 517, стр. A45. https://doi.org/0.1051/0004-6361/200912817

APA

Voshchinnikov, N. V., & Henning, T. (2010). From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe. ASTRONOMY & ASTROPHYSICS, 517, A45. https://doi.org/0.1051/0004-6361/200912817

Vancouver

Voshchinnikov NV, Henning T. From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe. ASTRONOMY & ASTROPHYSICS. 2010;517:A45. https://doi.org/0.1051/0004-6361/200912817

Author

Voshchinnikov, N.V. ; Henning, Th. / From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe. в: ASTRONOMY & ASTROPHYSICS. 2010 ; Том 517. стр. A45.

BibTeX

@article{28cf5ff56b6249cd87070366831a5c0f,
title = "From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe",
author = "N.V. Voshchinnikov and Th. Henning",
year = "2010",
doi = "0.1051/0004-6361/200912817",
language = "English",
volume = "517",
pages = "A45",
journal = "ASTRONOMY & ASTROPHYSICS",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - From interstellar abundances to grain composition: the major dust constituents Mg, Si, and Fe

AU - Voshchinnikov, N.V.

AU - Henning, Th.

PY - 2010

Y1 - 2010

U2 - 0.1051/0004-6361/200912817

DO - 0.1051/0004-6361/200912817

M3 - Article

VL - 517

SP - A45

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

ER -

ID: 5217003