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How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps? / Sobolev, A. M.; Cragg, D. M.; Ellingsen, S. P. et al.
In: Proceedings of the International Astronomical Union, Vol. 3, No. S242, 01.03.2007, p. 81-88.

Research output: Contribution to journalArticlepeer-review

Harvard

Sobolev, AM, Cragg, DM, Ellingsen, SP, Gaylard, MJ, Goedhart, S, Henkel, C, Kirsanova, MS, Ostrovskii, AB, Pankratova, NV, Shelemei, OV, Van Der Walt, DJ, Vasyunina, TS & Voronkov, MA 2007, 'How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?', Proceedings of the International Astronomical Union, vol. 3, no. S242, pp. 81-88. https://doi.org/10.1017/S1743921307012616

APA

Sobolev, A. M., Cragg, D. M., Ellingsen, S. P., Gaylard, M. J., Goedhart, S., Henkel, C., Kirsanova, M. S., Ostrovskii, A. B., Pankratova, N. V., Shelemei, O. V., Van Der Walt, D. J., Vasyunina, T. S., & Voronkov, M. A. (2007). How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps? Proceedings of the International Astronomical Union, 3(S242), 81-88. https://doi.org/10.1017/S1743921307012616

Vancouver

Sobolev AM, Cragg DM, Ellingsen SP, Gaylard MJ, Goedhart S, Henkel C et al. How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps? Proceedings of the International Astronomical Union. 2007 Mar 1;3(S242):81-88. doi: 10.1017/S1743921307012616

Author

Sobolev, A. M. ; Cragg, D. M. ; Ellingsen, S. P. et al. / How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?. In: Proceedings of the International Astronomical Union. 2007 ; Vol. 3, No. S242. pp. 81-88.

BibTeX

@article{8e92097684994b1e82f7b62b6cec10e7,
title = "How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?",
keywords = "Catalogs, Evolution, Galaxy: structure, ISM: clouds, Kinematics and dynamics, Masers, Radio lines: ISM, Stars: formation, Structure, Surveys",
author = "Sobolev, {A. M.} and Cragg, {D. M.} and Ellingsen, {S. P.} and Gaylard, {Michael J.} and Sharmila Goedhart and C. Henkel and Kirsanova, {M. S.} and Ostrovskii, {A. B.} and Pankratova, {N. V.} and Shelemei, {O. V.} and {Van Der Walt}, {D. J.} and Vasyunina, {T. S.} and Voronkov, {M. A.}",
year = "2007",
month = mar,
day = "1",
doi = "10.1017/S1743921307012616",
language = "English",
volume = "3",
pages = "81--88",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S242",

}

RIS

TY - JOUR

T1 - How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?

AU - Sobolev, A. M.

AU - Cragg, D. M.

AU - Ellingsen, S. P.

AU - Gaylard, Michael J.

AU - Goedhart, Sharmila

AU - Henkel, C.

AU - Kirsanova, M. S.

AU - Ostrovskii, A. B.

AU - Pankratova, N. V.

AU - Shelemei, O. V.

AU - Van Der Walt, D. J.

AU - Vasyunina, T. S.

AU - Voronkov, M. A.

PY - 2007/3/1

Y1 - 2007/3/1

KW - Catalogs

KW - Evolution

KW - Galaxy: structure

KW - ISM: clouds

KW - Kinematics and dynamics

KW - Masers

KW - Radio lines: ISM

KW - Stars: formation

KW - Structure

KW - Surveys

UR - http://www.scopus.com/inward/record.url?scp=38849189351&partnerID=8YFLogxK

U2 - 10.1017/S1743921307012616

DO - 10.1017/S1743921307012616

M3 - Article

AN - SCOPUS:38849189351

VL - 3

SP - 81

EP - 88

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S242

ER -

ID: 8912583