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Publications Based on SALT data Poland

Publications Based on SALT data Poland. OGLE-SMC-LPV00861 (LIN9) –the first proven Z And outburst in a Magellanic symbiotic star MNRAS letter submitted(Miszalski, Miko ł ajewska & Udalski).

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Publications Based on SALT data Poland

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  1. Publications Based on SALT data Poland

  2. OGLE-SMC-LPV00861 (LIN9) –the first proven Z And outburst in a Magellanic symbiotic star MNRAS letter submitted(Miszalski, Mikołajewska & Udalski)

  3. Miszalski, Brent; Mikołajewska, Joanna;"Identification of new Galactic symbiotic stars with SALT- I. Initial discoveries and other emission line objects"2014, Monthly Notices of the Royal Astronomical Society, Volume 440, Issue 2, p.1410-1419

  4. W. Narloch; J. Kaluzny; W. Krzeminski; W. Pych; M. Rozyczka; S. Shectman; I. B. Thompson; and T. Tomov;"New observations of the old magnetic nova GQ Muscae" 2014, Baltic Astronomy, vol. 23, 1-7 The spectrum of GQ Mus from April 2012 smoothed with a 9-pixel moving box Evidence of the presence of magnetic field – polar.

  5. Hajduk, M.; Gładkowski, M.; Soszyński, I.;"Search for binary central stars of the SMC Pne"2014, Astronomy & Astrophysics, Volume 561, id.A8, 7 pp. Spectra of the variable objects Used to constrain the nature of the objects or search for additional evidence for binarity.

  6. Hryniewicz, K.; Czerny, B.; Pych, W.; Udalski, A.; Krupa, M.; Świȩtoń, A.; Kaluzny, J.;"SALT long-slit spectroscopy of LBQS 2113-4538:variability of the Mg II and Fe II component"2014, Astronomy & Astrophysics, Volume 562, id.A34 Best fit and residuals for the Tsuzuki et al. Fe II template and the two-Gaussian model for Mg II LBQS 2113-4538 Model of the spectrum and variability analysis.

  7. Gałan, C.; Tomov, T.; Kato, T.; Pojmański, G.; Szczygieł, D. M.; Pilecki, B.; Graczyk, D.; Gromadzki, M.; Mikołajewski, M.; Gieren, W.; Strobel, A.; Roukema, B. F."A new look at the long-period eclipsing binary V383 Scorpi" 2013, Astronomy & Astrophysics, Volume 550, id.A93, 13 pp. Observed low-resolution spectrum of V383 Sco (thick line) compared with the model (thin line)that is a superposition of F0 and M1 supergiant spectra (grey lines). Determination of spectral types of the components.

  8. Zola, S.; Zejda, M.; Siwak, M.; de Villiers, S. N., "Rediscussion of the Early Type Eclipsing Binary SV Cen" 2013, Central European Astrophysical Bulletin, p. 79-84 Six spectra of SV Cen taken at the secondary minimum. Complex variability of the spectrum.

  9. Ulusoy, C.; Niemczura, E.; Ulaş, B.; Gülmez, T."New β Cephei variable in the Southern open clusterNGC 6200: ALS 3728"2013, New Astronomy, Volume 23, p. 55-58. Observed (black) and synthetic (red-fitted) spectra of ALS 3728 for selected regions. Spectra used for determination of the parameters of the stellar atmosphere.

  10. Ulusoy, C.; Niemczura, E.; Ulaş, B.; Gülmez, T."An asteroseismic study of the Southern β Cephei star ALS 3721"2013, New Astronomy, Volume 22, p. 51-56. Observed (black) and synthetic (red-fitted) spectra of ALS 3721 for selected regions. Spectra used for determination of the parameters of the stellar atmosphere.

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