We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TUBITAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables; 17 periods are identified for the first time. Crown Copyright
We have observed a sample of δ Scuti stars discovered by the ROTSE collaboration in 1999 with Supe...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
We have observed a sample of δ Scuti stars discovered by the ROTSE collaboration in 1999 with Supe...
We have studied the long-term variations of Mira type variables observed with Robotic Optical Transi...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecraft have been analysed t...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
We present here the results and interpretation of a long-term OH variability program conducted with...
The variability of several stars shows "Mira-type" and "semiregular" behavior during long-time data ...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
International audienceContext. Variability is a key property of stars on the asymptotic giant branch...
International audienceContext. Variability is a key property of stars on the asymptotic giant branch...
The present uvby data, IUE FES measurements and American Association of Variable Star Observers visu...
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB) phase of...
Abstract. A program of UBV (RI)c photometric ob-servations of twelve southern hemisphere Long Period...
International audienceContext. Variability is a key property of stars on the asymptotic giant branch...
We have observed a sample of δ Scuti stars discovered by the ROTSE collaboration in 1999 with Supe...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
We have observed a sample of δ Scuti stars discovered by the ROTSE collaboration in 1999 with Supe...
We have studied the long-term variations of Mira type variables observed with Robotic Optical Transi...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecraft have been analysed t...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
We present here the results and interpretation of a long-term OH variability program conducted with...
The variability of several stars shows "Mira-type" and "semiregular" behavior during long-time data ...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
International audienceContext. Variability is a key property of stars on the asymptotic giant branch...
International audienceContext. Variability is a key property of stars on the asymptotic giant branch...
The present uvby data, IUE FES measurements and American Association of Variable Star Observers visu...
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB) phase of...
Abstract. A program of UBV (RI)c photometric ob-servations of twelve southern hemisphere Long Period...
International audienceContext. Variability is a key property of stars on the asymptotic giant branch...
We have observed a sample of δ Scuti stars discovered by the ROTSE collaboration in 1999 with Supe...
Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed ...
We have observed a sample of δ Scuti stars discovered by the ROTSE collaboration in 1999 with Supe...