The highly polarized open cluster trumpler 27
We have carried out multicolor linear polarimetry (U BV RI) of the brightest stars in the area of the open cluster Trumpler 27. Our data show a high level of polarization in the stellar light with a considerable dispersion, from P = 4% to P = 9.5%. The polarization vectors of the cluster members app...
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2000
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v120_n4_p1906_Feinstein http://hdl.handle.net/20.500.12110/paper_00046256_v120_n4_p1906_Feinstein |
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paper:paper_00046256_v120_n4_p1906_Feinstein2023-06-08T14:27:11Z The highly polarized open cluster trumpler 27 Dust, extinction Open clusters and associations: individual (Trumpler 27) We have carried out multicolor linear polarimetry (U BV RI) of the brightest stars in the area of the open cluster Trumpler 27. Our data show a high level of polarization in the stellar light with a considerable dispersion, from P = 4% to P = 9.5%. The polarization vectors of the cluster members appear to be aligned. Foreground polarization was estimated from the data of some nonmember objects, for which two different components were resolved: the first one associated with a dust cloud close to the Sun producing Pλmax = 1.3% and θ = 146°, and a second component, the main source of polarization for the cluster members, originating in another dust cloud, which polarizes the light in the direction of θ = 29°.5. From a detailed analysis, we found that the two components have associated values EB-V < 0.45 for the first one and EB-V > 0.75 for the other. Due the difference in the orientation of both polarization vectors, almost 90° (180° at the Stokes representation), the first cloud (θ ∼ 146°) depolarizes the light strongly polarized by the second one (θ ∼ 29°.5). 2000 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v120_n4_p1906_Feinstein http://hdl.handle.net/20.500.12110/paper_00046256_v120_n4_p1906_Feinstein |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Dust, extinction Open clusters and associations: individual (Trumpler 27) |
| spellingShingle |
Dust, extinction Open clusters and associations: individual (Trumpler 27) The highly polarized open cluster trumpler 27 |
| topic_facet |
Dust, extinction Open clusters and associations: individual (Trumpler 27) |
| description |
We have carried out multicolor linear polarimetry (U BV RI) of the brightest stars in the area of the open cluster Trumpler 27. Our data show a high level of polarization in the stellar light with a considerable dispersion, from P = 4% to P = 9.5%. The polarization vectors of the cluster members appear to be aligned. Foreground polarization was estimated from the data of some nonmember objects, for which two different components were resolved: the first one associated with a dust cloud close to the Sun producing Pλmax = 1.3% and θ = 146°, and a second component, the main source of polarization for the cluster members, originating in another dust cloud, which polarizes the light in the direction of θ = 29°.5. From a detailed analysis, we found that the two components have associated values EB-V < 0.45 for the first one and EB-V > 0.75 for the other. Due the difference in the orientation of both polarization vectors, almost 90° (180° at the Stokes representation), the first cloud (θ ∼ 146°) depolarizes the light strongly polarized by the second one (θ ∼ 29°.5). |
| title |
The highly polarized open cluster trumpler 27 |
| title_short |
The highly polarized open cluster trumpler 27 |
| title_full |
The highly polarized open cluster trumpler 27 |
| title_fullStr |
The highly polarized open cluster trumpler 27 |
| title_full_unstemmed |
The highly polarized open cluster trumpler 27 |
| title_sort |
highly polarized open cluster trumpler 27 |
| publishDate |
2000 |
| url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v120_n4_p1906_Feinstein http://hdl.handle.net/20.500.12110/paper_00046256_v120_n4_p1906_Feinstein |
| _version_ |
1768546655379914752 |