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The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm. / Samodurov, V. A.; Volvach, A. E.; Siparov, S. V. и др.
ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: 4th Gamow International Conference on Astrophysics and Cosmology after Gamow and the 9th Gamow Summer School. ред. / S. K. Chakrabarti; G. BisnovatyiKogan; A. I. Zhuk. Том 1206 USA: American Institute of Physics Inc., 2009. стр. 346-353 (AIP Conference Proceedings; Том 1206).

Результаты исследований: Глава в книге, отчете, сборнике статей › Материалы конференции › Рецензирование

Harvard

Samodurov, VA, Volvach, AE, Siparov, SV, Tolmachev, AM, Rudnitskij, GM, Volvach, LN, Subaev, IA, Logvinenko, SV & Ladejshchikov, DA 2009, The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm. в SK Chakrabarti, G BisnovatyiKogan & AI Zhuk (ред.), ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: 4th Gamow International Conference on Astrophysics and Cosmology after Gamow and the 9th Gamow Summer School. Том. 1206, AIP Conference Proceedings, Том. 1206, American Institute of Physics Inc., USA, стр. 346-353. https://doi.org/10.1063/1.3292539

APA

Samodurov, V. A., Volvach, A. E., Siparov, S. V., Tolmachev, A. M., Rudnitskij, G. M., Volvach, L. N., Subaev, I. A., Logvinenko, S. V., & Ladejshchikov, D. A. (2009). The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm. в S. K. Chakrabarti, G. BisnovatyiKogan, & A. I. Zhuk (Ред.), ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: 4th Gamow International Conference on Astrophysics and Cosmology after Gamow and the 9th Gamow Summer School (Том 1206, стр. 346-353). (AIP Conference Proceedings; Том 1206). American Institute of Physics Inc.. https://doi.org/10.1063/1.3292539

Vancouver

Samodurov VA, Volvach AE, Siparov SV, Tolmachev AM, Rudnitskij GM, Volvach LN и др. The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm. в Chakrabarti SK, BisnovatyiKogan G, Zhuk AI, Редакторы, ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: 4th Gamow International Conference on Astrophysics and Cosmology after Gamow and the 9th Gamow Summer School. Том 1206. USA: American Institute of Physics Inc. 2009. стр. 346-353. (AIP Conference Proceedings). doi: 10.1063/1.3292539

Author

Samodurov, V. A. ; Volvach, A. E. ; Siparov, S. V. и др. / The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm. ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: 4th Gamow International Conference on Astrophysics and Cosmology after Gamow and the 9th Gamow Summer School. Редактор / S. K. Chakrabarti ; G. BisnovatyiKogan ; A. I. Zhuk. Том 1206 USA : American Institute of Physics Inc., 2009. стр. 346-353 (AIP Conference Proceedings).

BibTeX

@inproceedings{76ae450248db4c6598d86f12ca91f276,
title = "The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm",
abstract = "Results of a search for ultra rapid flux fluctuations of galactic sources of maser emission in the water-vapor line at a wavelength of 1.35 cm. An observational technique of a search for ultra rapid flux fluctuations has been developed. From 2002 to 2009 a number of observational sessions for about 40 maser sources have been carried out. Several of them have demonstrated such a variability. Possible mechanisms of the variability are discussed, among them internal processes within the sources themselves as well as external ones, including the theoretical possibility of a resonant effect of gravitational waves from galactic objects on the maser region. Clear evidence for the presence of such a variability has been found in several sources (Cep A, W43M3, W49N, W33B). This variability appears not permanently, but only certain states of particular H2O masers. In some sources (Ori A, W3 OH, W49N) demonstrated any variations by linear polarization of signal. For the Russian authors this work was supported by the Russian Foundation for Basic Research (08-02-01179).",
author = "Samodurov, {V. A.} and Volvach, {A. E.} and Siparov, {S. V.} and Tolmachev, {A. M.} and Rudnitskij, {G. M.} and Volvach, {L. N.} and Subaev, {I. A.} and Logvinenko, {S. V.} and Ladejshchikov, {D. A.}",
note = "The authors gratefully acknowledge the support from the Russian Foundation for Basic Research (project codes 08-02-01179).",
year = "2009",
doi = "10.1063/1.3292539",
language = "English",
isbn = "978-0-7354-0743-5",
volume = "1206",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics Inc.",
pages = "346--353",
editor = "Chakrabarti, {S. K. } and BisnovatyiKogan, {G. } and Zhuk, {A. I. }",
booktitle = "ASTROPHYSICS AND COSMOLOGY AFTER GAMOW",
address = "United States",

}

RIS

TY - GEN

T1 - The results of ultra‐rapid flux fluctuations monitoring in 2002–2009 for galactic sources of water‐vapor maser emission at a wavelength of 1.35 cm

AU - Samodurov, V. A.

AU - Volvach, A. E.

AU - Siparov, S. V.

AU - Tolmachev, A. M.

AU - Rudnitskij, G. M.

AU - Volvach, L. N.

AU - Subaev, I. A.

AU - Logvinenko, S. V.

AU - Ladejshchikov, D. A.

N1 - The authors gratefully acknowledge the support from the Russian Foundation for Basic Research (project codes 08-02-01179).

PY - 2009

Y1 - 2009

N2 - Results of a search for ultra rapid flux fluctuations of galactic sources of maser emission in the water-vapor line at a wavelength of 1.35 cm. An observational technique of a search for ultra rapid flux fluctuations has been developed. From 2002 to 2009 a number of observational sessions for about 40 maser sources have been carried out. Several of them have demonstrated such a variability. Possible mechanisms of the variability are discussed, among them internal processes within the sources themselves as well as external ones, including the theoretical possibility of a resonant effect of gravitational waves from galactic objects on the maser region. Clear evidence for the presence of such a variability has been found in several sources (Cep A, W43M3, W49N, W33B). This variability appears not permanently, but only certain states of particular H2O masers. In some sources (Ori A, W3 OH, W49N) demonstrated any variations by linear polarization of signal. For the Russian authors this work was supported by the Russian Foundation for Basic Research (08-02-01179).

AB - Results of a search for ultra rapid flux fluctuations of galactic sources of maser emission in the water-vapor line at a wavelength of 1.35 cm. An observational technique of a search for ultra rapid flux fluctuations has been developed. From 2002 to 2009 a number of observational sessions for about 40 maser sources have been carried out. Several of them have demonstrated such a variability. Possible mechanisms of the variability are discussed, among them internal processes within the sources themselves as well as external ones, including the theoretical possibility of a resonant effect of gravitational waves from galactic objects on the maser region. Clear evidence for the presence of such a variability has been found in several sources (Cep A, W43M3, W49N, W33B). This variability appears not permanently, but only certain states of particular H2O masers. In some sources (Ori A, W3 OH, W49N) demonstrated any variations by linear polarization of signal. For the Russian authors this work was supported by the Russian Foundation for Basic Research (08-02-01179).

UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000281437400029

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=77951811895

U2 - 10.1063/1.3292539

DO - 10.1063/1.3292539

M3 - Conference contribution

SN - 978-0-7354-0743-5

VL - 1206

T3 - AIP Conference Proceedings

SP - 346

EP - 353

BT - ASTROPHYSICS AND COSMOLOGY AFTER GAMOW

A2 - Chakrabarti, S. K.

A2 - BisnovatyiKogan, G.

A2 - Zhuk, A. I.

PB - American Institute of Physics Inc.

CY - USA

ER -

ID: 38842269