MASYS. The AKARI spectroscopic survey of Symbiotic Stars in the Magellanic Clouds
R. Angeloni (1,2), S. Ciroi (1), P. Marigo (1), M. Contini (2,1), F., Di Mille (1), and P. Rafanelli (1) - ((1) Department of Astronomy, University, of Padova, Italy; (2) School of Physics & Astronomy, Tel Aviv University,, Israel)
TL;DR
MASYS is a pioneering AKARI survey providing the first near-infrared spectra of extragalactic symbiotic stars in the Magellanic Clouds, enhancing understanding of these complex stellar systems.
Contribution
It presents the first near-IR spectroscopic data of extragalactic symbiotic stars, expanding the observational database for these objects in the Magellanic Clouds.
Findings
First near-IR spectra of extragalactic symbiotic stars obtained
Data will improve understanding of symbiotic star properties in external galaxies
Survey is part of a major European observational program
Abstract
MASYS is the AKARI spectroscopic survey of Symbiotic Stars in the Magellanic Clouds, and one of the European Open Time Observing Programmes approved for the AKARI (Post-Helium) Phase-3. It is providing the first ever near-IR spectra of extragalactic symbiotic stars. The observations are scheduled to be completed in July 2009.
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies