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The Optical Gravitational Lensing Experiment. Catalog of High Proper Motion Stars Towards the Magellanic Clouds

Wybrane pełne teksty z tego czasopisma
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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
We present a Catalog of high proper motion (HPM) stars detected in the foreground of central parts of the Magellanic Clouds. The Catalog contains 2161 objects in the 4.5 square degree area towards the LMC, and 892 HPM stars in the 2.4 square degree area towards the SMC. The Catalog is based on observations collected during four years of the OGLE-II microlensing survey. The Difference Image Analysis (DIA) of the images provided candidate HPM stars with proper motion as small as 4 mas/yr. These appeared as pseudo-variables, and were all measured astrometrically on all CCD images, providing typically about 400 data points per star. The reference frame was defined by the majority of background stars, most of them members of the Magellanic Clouds. The reflex motion due to solar velocity with respect to the local standards of rest is clearly seen. The largest proper motion in our sample is 363 mas/yr. Parallaxes were measured with errors smaller than 20% for several stars.
Słowa kluczowe
Czasopismo
Rocznik
Strony
129--142
Opis fizyczny
Bibliogr. 21 poz., rys., tab., wykr., zdj.
Twórcy
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • Los Alamos National Observatory, MS-D436, Los Alamos NM 85745, USA
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • Universidad de Concepción, Departamento de Fisica, Casilla 160-C, Concepción, Chile
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
Bibliografia
  • Alard, C. 2000, Astron. Astrophys. Suppl. Ser., 144, 363.
  • Alcock, C., et al. 2001, Astrophys. J., 562, 337.
  • Dehnen, W., and Binney, J.J. 1998, MNRAS, 298, 387.
  • Eyer, L., and Woźniak, P.R. 2001, MNRAS, 327, 601.
  • Gould, A. 2000, Astrophys. J., 532, 936.
  • Luyten, W. J. 1979, "New Luyten Catalogue of Stars with ProperMotions Larger than Two Tenths of an Arcsecond" (Minneapolis: Univ. Minnesota Press).
  • Luyten, W.J., and Hughes, H.S. 1980, "Proper Motion Survey with the Forty Eight Inch Schmidt Telescope, First Supplement to the NLTT" (Minneapolis: Univ. Minnesota Press).
  • Nelson, C.A., Cook, K.H., Axelrod, T.S., Mould, J.R., and Alcock C. 2001, Astrophys. J., 573, 644.
  • Oppenheimer, B.R., Hambly, N.C., Digby, A.P., Hodgkin, S.T., and Saumon, D. 2001, Science, 292, 698.
  • Paczyński, B. 1996, Acta Astron., 46, 291.
  • Paczyński, B. 1998, Astrophys. J. Letters, 494, L23.
  • Perryman, M.A.C., et al. 1997, Astron. Astrophys., 323, L49.
  • Salim, S., and Gould, A. 2000, Astrophys. J., 539, 241.
  • Schechter, P.L.,Mateo, M.L., and Saha, A. 1993, P.A.S.P., 105, 1342.
  • Scholz, R.D., Irwin, M., Ibata, R., Jahreiss, H., and Malkov, O.Yu. 2000, Astron. Astrophys., 353, 958.
  • Udalski, A., Kubiak, M., and Szymański, M. 1997, Acta Astron., 47, 319.
  • Udalski, A., Szymański, M., Kubiak, M., Pietrzyński, G., Woźniak, P.R., and Żebruń, K. 1998, Acta Astron., 48, 147.
  • van Flandern, and T.C., Pulkkinen, K.F. 1979, Astrophys. J. Suppl. Ser., 41, 391.
  • Woźniak, P.R. 2000, Acta Astron., 50, 421.
  • Wroblewski, H., and Costa E. 2001, Astron. Astrophys., 367, 725.
  • Żebruń, K., Soszyński, I., and Woźniak, P. R. 2001, Acta Astron., 51, 303.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-bcecb573-e6d3-4bba-affb-05f816bd5d60
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