dc.creatorEVGUENI LEKHT EVGUENIEVICH
dc.date2008
dc.date.accessioned2023-07-25T16:22:53Z
dc.date.available2023-07-25T16:22:53Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1049
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7806249
dc.descriptionThe results of analyzing asymmetry in the H₂O maser lines at λ = 1.35 cm are presented. We investigated in detail the known mechanism of the asymmetry origin due to the hyperfine structure of the 6₁₆ → 5₂₃ transition and different (not equidistant) positions of the corresponding triplet components. The triplet of the lines is characterized by the sum of extinction factors that are continuously transformed into a single-peaked asymmetric extinction coefficient, with the increase in the Doppler widths (characterizing by effective Doppler velocity ud). A noticeable asymmetry corresponds to ud ≤ 0.5−1 km s¯¹. For higher values of ud the extinction factor approaches a Gaussian shape with the decreasing magnitude of the profile asymmetry. An appreciable asymmetry in unsaturated maser lines can only arise at ud ≤ 0.5 km s¯¹, if there are very narrow linewidths (Δu ≈ 0.2−0.4 km s¯¹). But observed saturated masers possess a fairly high degree of the line asymmetry, 10−40%. Most probably, this asymmetry is a result of rebroadening of the linewidth up to the value that is comparable to the width of the asymmetric extinction coefficient.
dc.formatapplication/pdf
dc.languageeng
dc.publisherAstronomy and Astrophysics
dc.relationcitation:Lekht, E. E., et al., (2008). A study of the asymmetry in the H₂O maser line at λ = 1.35 cm on the base of the hyperfine structure, Astronomy and Astrophysics, Vol.492(2):475-480
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleA study of the asymmetry in the H₂O maser line at λ = 1.35 cm on the base of the hyperfine structure
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


Este ítem pertenece a la siguiente institución