Multicolor polarimetry of stars in the open cluster Trumpler 27

Observations of multicolor polarimetry of the stars in the region of the open cluster Trumpler 27 have been obtained at CASLEO, San Juan, Argentina. These data show rather high values of polarization but with a considerable scatter (P ∼ 4% to 9.5%). On the other hand, the angle of the polarimetric v...

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Detalles Bibliográficos
Autor principal: Baume, G.
Otros Autores: Feinstein, C., Vázquez, R.A, Niemela, V.S, Cerruti, M.A
Formato: Acta de conferencia Capítulo de libro
Lenguaje:Inglés
Publicado: 1999
Acceso en línea:Registro en Scopus
Handle
Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
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100 1 |a Baume, G. 
245 1 0 |a Multicolor polarimetry of stars in the open cluster Trumpler 27 
260 |c 1999 
270 1 0 |m Baume, G.; Observatorio Astronómico, Paseo del Bosque, 1900 La Plata, Argentina; email: gbaume@fcaglp.fcaglp.unlp.edu.ar 
506 |2 openaire  |e Política editorial 
504 |a Bakker, R., Thé, P.S., (1983) A&AS, 52, p. 27 
504 |a Baume, G., Feinstein, C., Vázquez, R.A., (1999), in preparation; Moffat, A.F.J., FitzGerald, M.P., Jackson, P.D., (1977) ApJ, 215, p. 106 
504 |a Serkowski, K. 1971, in IAU Symp. No. 52, Interstellar Dust and Related Topics, ed. J. M. Greenberg & H. C. van den Hulst (Dordrecht: Reidel), 144; Thé, P.S., Stokes, N., (1970) A&A, 5, p. 298 
504 |a Whittet, D.C.B., Martin, P.G., Hough, J.H., Rouse, M.F., Bailey, J.A., Axon, D.J., (1992) ApJ, 386, p. 562 
520 3 |a Observations of multicolor polarimetry of the stars in the region of the open cluster Trumpler 27 have been obtained at CASLEO, San Juan, Argentina. These data show rather high values of polarization but with a considerable scatter (P ∼ 4% to 9.5%). On the other hand, the angle of the polarimetric vectors appears to be constant in the sample. A new numerical algorithm is used to study the different components of the observed polarization vectors. We estimate the foreground polarization vector of the cluster from observations of a few foreground, non-member stars seen in the region. Our data suggest that a patchy dust structure is present across the cluster surface. © Universidad Nacional Autónoma de México.  |l eng 
593 |a Observatorio Astronómico, Paseo del Bosque, 1900 La Plata, Argentina 
593 |a Instituto de Astronomía Y Física del Espacio, CC 67, Suc. 28, 1428 Buenos Aires, Argentina 
593 |a CONICET, Argentina 
593 |a CIC, Prov. Buenos Aires, Argentina 
690 1 0 |a ISM: DUST, EXTINCTION 
690 1 0 |a OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL (TRUMPLER 27) 
690 1 0 |a POLARIMETRY 
700 1 |a Feinstein, C. 
700 1 |a Vázquez, R.A. 
700 1 |a Niemela, V.S. 
700 1 |a Cerruti, M.A. 
711 2 |c La Plata  |d 1 December 1997 through 5 December 1997 
773 0 |d 1999  |g v. 8  |h pp. 79-81  |p Rev.Mex. Astron. Astrofis. Ser. Conf.  |n Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias  |x 14052059  |w (AR-BaUEN)CENRE-1052  |t Workshop on Hot Stars in Open Clusters of the Galaxy and the Magellanic Clouds 
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856 4 0 |u https://hdl.handle.net/20.500.12110/paper_14052059_v8_n_p79_Baume  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v8_n_p79_Baume  |y Registro en la Biblioteca Digital 
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