Oxygen and carbon rich cool stars in the Cepheus region: classification of selected objects from KP2001 catalogue. I |
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Authors: | C. Rossi S. Gaudenzi G. V. Petrosyan R. Nesci S. Sclavi |
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Affiliation: | (1) Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-stra e 1, D-85748 Garching, Germany;(2) South African Astronomical Obsevatory, P.O. Box 9, 7935 Observatory, South Africa;(3) Dept. of Physics, University College, ADFA, Canberra, ACT, 2600, Australia;(4) Institut für Astronomie der Universität Wien, Türkenschanzstra e 17, A-1180 Wien, Austria |
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Abstract: | We present moderate resolution CCD spectra and R photometry for seven KP2001 stars. We revised the spectral classification of the stars in the range λλ4000−8700? . Our photometric data confirmed the behavior of the light curves downloaded from the NSVS (Northern Sky Variability Survey) database. For KP2001-32, presented as a Mira-type variable in NSVS, we estimated absolute bolometric M b and K-band M K magnitudes as well as the distance using the period-luminosity relations. We also estimated the mass loss rate using the calibration relations between mass loss rate and K - [12] index. From the position in infrared color-color diagrams, we confirmed the photometric classification of KP2001-221 as a semiregular variable, based on the light curve of the NSVS database. For the N-type carbon star KP2001-77 we estimated distance and absolute magnitude M K using different calibration methods. For the remaining four objects we derived the absolute magnitudes and distances using our CCD spectra and published JHK S magnitudes. We discuss the nature of these objects on the basis of the obtained results. |
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