2008Unpublished venueRequires access

Radial Velocity Measurements for Pulsating Stars with Poznan Spectroscopic Telescope: First Results

Agata Rożek, R. Baranowski, P. Bartczak, W. Borczyk, W. Dimitrov, M. Fagas, K. Kamínski, T. Kwiatkowski, R. Ratajczak, A. Schwarzenberg-Czerny

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Abstract

We present examples of radial velocity measurements obtained with the Poznan Spectroscopic Telescope (PST). Observations on PST are run on regular basis since August 2007. The PST is a binary telescope with two 40 cm mirrors of a Newtonian focus, connected by optic fibers with an echelle spectrograph. Radial velocity measurements are done for δ Sct, β Cep, classical Cepheids, eclipsing binaries and other types of variable stars. Echelle spectra reduction and radial velocity measurements are performed with IRAF package. Final results are obtained from cross-correlating stellar spectra either with radial velocity standards or the program star itself using IRAF fxcor procedure.

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What this paper is about

We present examples of radial velocity measurements obtained with the Poznan Spectroscopic Telescope (PST). Observations on PST are run on regular basis since August 2007. The PST is a binary telescope with two 40 cm mirrors of a Newtonian focus, connected by optic fibers with an echelle spectrograph. Radial velocity measurements are done for δ Sct, β Cep, classical Cepheids, eclipsing binaries and other types of variable stars. Echelle spectra reduction and radial velocity measurements are performed with IRAF package. Final results are obtained from cross-correlating stellar spectra either with radial velocity standards or the program star itself using IRAF fxcor procedure.

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Available abstract

We present examples of radial velocity measurements obtained with the Poznan Spectroscopic Telescope (PST). Observations on PST are run on regular basis since August 2007. The PST is a binary telescope with two 40 cm mirrors of a Newtonian focus, connected by optic fibers with an echelle spectrograph. Radial velocity measurements are done for δ Sct, β Cep, classical Cepheids, eclipsing binaries and other types of variable stars. Echelle spectra reduction and radial velocity measurements are performed with IRAF package. Final results are obtained from cross-correlating stellar spectra either with radial velocity standards or the program star itself using IRAF fxcor procedure.

Key concepts: Radial velocity, Physics, Astrophysics, Spectrograph, Cepheid variable, Telescope, Binary star, Stars

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