Παρακαλούμε σημειώστε ότι σε περίπτωση δημοσίευσης άρθρου που χρησιμοποιεί τα δεδομένα του Αρίσταρχου θα πρέπει να ακολουθείτε τις παρακάτω οδηγίες:
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Credit “Aristarchos telescope” in published papers:
Publications based wholly or in part on data obtained at the Aristarchos telescope are required to carry the following Acknowledgment, primarily as a footnote to the title but, if such footnotes are not permitted by the journal, book, etc, then in the Acknowledgments section of the paper itself:
“Based on observations made with the 2.3m Aristarchos telescope, Helmos Observatory, Greece, which is operated by the Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing of the National Observatory of Athens, Greece.”
Πρόσφατες Δημοσιεύσεις
A Study of Nine Extremely Low Mass Ratio-contact Binary Systems
Ramos-Larios G., Guerrero M. A., Toalá J. A., Akras S., Fang X.
H2 molecular gas in the old planetary nebula NGC 3587
Ramos-Larios G., Guerrero M. A., Toalá J. A., Akras S., Fang X.
A Unique Low-mass-ratio Contact Eclipsing Binary System under the Period Cutoff
Papageorgiou, Athanasios ; Christopoulou, Panagiota-Eleftheria
Three Ultra-short-period Contact Eclipsing Binary Systems Mined from Massive Astronomical Surveys
Papageorgiou, A., Christopoulou, P.-E., Ferreira
Asteroid spin-states of a 4 Gyr collisional family
Athanasopoulos, D., Hanuš, J., Avdellidou,
CoBiToM Project — II: Evolution of contact binary systems close to the orbital period cut-off
Loukaidou, G. A. ; Gazeas,
Discovery of an optical cocoon tail behind the runaway HD 185806
Studies on the circumstellar structures around evolved stars provide vital information on the evolution of the parent star and the properties of the local interstellar medium. In this work, we present the discovery and characterization of an optical cocoon tail behind the star HD 185806. The cocoon apex emission is puzzling, as it is detected in the infrared but shows no signal in the optical wavelength.