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dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorBarbuy, Beatrizpt_BR
dc.contributor.authorMomany, Yazanpt_BR
dc.date.accessioned2014-07-24T02:04:23Zpt_BR
dc.date.issued2002pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98515pt_BR
dc.description.abstractPismis 23 and Stephenson 2 are two very reddened open clusters, projected close to the Galactic plane. We present VI and JH photometry for Pismis 23 and I and Gunn z for Stephenson 2. We derive a relatively old age of ~ 700 Myr for Pismis 23, with a reddening value of E(B−V) = 1:73 and a distance dʘ ≈ 2.6 kpc from the Sun. Stephenson 2 has a clump of red supergiants, indicating a young age of about 20 Myr, somewhat younger and more distant (dʘ ≈ 6 kpc) than recently reported in the literature. The age estimate for such a young object is crucial for the distance estimate. The high reddening of these two clusters relative to predictions from the di use interstellar medium at their distances is due to discrete intervening clouds.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and astrophysics. Les Ulis. Vol. 390, no. 3 (Aug. 2002), p. 931-935pt_BR
dc.rightsOpen Accessen
dc.subjectFotometria astronômicapt_BR
dc.subjectOpen clusters and associations: individual: Pismis 23, Stephenson 2en
dc.subjectAstronomia infravermelhapt_BR
dc.subjectStars: Hertzsprung-Russell (HR) and C-M diagramsen
dc.subjectAglomerados estelarespt_BR
dc.subjectEstrelas supergigantespt_BR
dc.titleThe very reddened open clusters Pismis 23 (Lynga 10) and Stephenson 2pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000327575pt_BR
dc.type.originEstrangeiropt_BR


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