Search Results - "Samsonyan, A."

Analysis of Emission Line Widths of [CII] 158μm by Samsonyan, A. L.

“…A study of [CII] 158 μm emission line profiles observed with Herschel PACS for 379 galaxies is presented. Emission line widths are compared to [CII]…”
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STAR FORMATION RATES FROM [C II] 158 μm AND MID-INFRARED EMISSION LINES FOR STARBURSTS AND ACTIVE GALACTIC NUCLEI by Sargsyan, L, Samsonyan, A, LeBouteiller, V, Weedman, D, Barry, D, Bernard-Salas, J, Houck, J, Spoon, H

“…A summary is presented for 130 galaxies observed with the Herschel Photodetector Array Camera and Spectrometer instrument to measure fluxes for the [CII] 158…”
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New eruptive variable(s) in the RAFGL 7009S H ii region by Nikoghosyan, E H, Azatyan, N M, Andreasyan, D H, Kaper, L, Samsonyan, A L, Yeghikyan, A G, Baghdasaryan, D S, Harutyunyan, N A

“…ABSTRACT Eruptions of young stellar objects (YSOs) are rare events, therefore a new outburst is always noteworthy. We present two new high-amplitude variable…”
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[C II] 158 μm LUMINOSITIES AND STAR FORMATION RATE IN DUSTY STARBURSTS AND ACTIVE GALACTIC NUCLEI by Sargsyan, L, LeBouteiller, V, Weedman, D, Spoon, H, Bernard-Salas, J, Engels, D, Stacey, G, Houck, J, Barry, D, Miles, J, Samsonyan, A

“…Results are presented for [CII] 158 mu m line fluxes observed with the Herschel PACS instrument in 112 sources with both starburst and active galactic nucleus…”
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Variation in the flare activity of the star UV Ceti by Melikian, N. D., Tamazian, V. S., Samsonyan, A. L.

“…This is an analysis of the dependence of the flare activity of the well known flare star UV Ceti on the linear distance between the components of this binary…”
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Emission stars in Cyg OB7. new flare stars. III by Melikian, N. D., Tamazian, V. S., Karapetian, A. A., Samsonyan, A. L.

“…A continued search for emission objects in three new fields within the association Cyg OB7 yielded eight new emission stars in one of these fields. No emission…”
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Dust obscuration of the narrow line region of active galactic nuclei by Sargsyan, L., Gevorgyan, M., Abrahamyan, H. V., Kostandyan, G., Paronyan, G., Samsonyan, A., Sargsyan, D., Sinamyan, P.

“…To estimate the dust absorption of the Narrow Line Region (NLR) of AGN, we have compared the infrared [NeIII] 15.55 μm line and optical [OIII] 5007 Å line…”
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The runaway nature and origin of {\alpha} Crucis system by Torosyan, M, Azatyan, N, Nikoghosyan, E, Samsonyan, A, Andreasyan, D

“…Massive stars are always the focus of astronomical research and a significant part of them (10--20%) moves in space at a high (supersonic) velocity. This paper…”
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Searching for stellar population in the molecular cloud GRSMC 045.49+00.04 by Azatyan, N, Nikoghosyan, E, Samsonyan, A, Elia, D, Kaper, L, Yeghikyan, A, Andreasyan, D, Baghdasaryan, D

“…Understanding the characteristics of young stellar populations is essential for deriving insights into star formation processes within parent molecular clouds…”
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[CII] 158 micron Luminosities and Star Formation Rate in Dusty Starbursts and AGN by Sargsyan, L, Lebouteiller, V, Weedman, D, Spoon, H, Bernard-Salas, J, Engels, D, Stacey, G, Houck, J, Barry, D, Miles, J, Samsonyan, A

“…Results are presented for [CII] 158 micron line fluxes observed with the Herschel PACS instrument in 112 sources with both starburst and AGN classifications,…”
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