Vampire Star Reveals Its Secrets
Astronomers have obtained the best images ever of a star that has lost most of its material to a vampire companion. By combining the light captured by four telescopes at ESO´s Paranal Observatory they created a virtual telescope 130 meters across with vision 50 times sharper than the NASA/ESA Hubble Space Telescope. Surprisingly, the new results show that the transfer of mass from one star to the other in this double system is gentler than expected.
“We can now combine light from four VLT telescopes and create super-sharp images much more quickly than before,” says Nicolas Blind (IPAG, Grenoble, France), who is the lead author on the paper presenting the results, “The images are so sharp that we can not only watch the stars orbiting around each other, but also measure the size of the larger of the two stars.”
The astronomers observed  the unusual system SS Leporis in the constellation of Lepus (The Hare), which contains two stars that circle around each other in 260 days. The stars are separated by only a little more than the distance between the Sun and the Earth, while the largest and coolest of the two stars extends to one quarter of this distance – corresponding roughly to the orbit of Mercury. Because of this closeness, the hot companion has already cannibalized about half of the mass of the larger star.
“We knew that this double star was unusual, and that material was flowing from one star to the other,” says co-author Henri Boffin, from ESO. “What we found, however, is that the way in which the mass transfer most likely took place is completely different from previous models of the process. The ℠bite´ of the vampire star is very gentle but highly effective.”
The new observations are sharp enough to show that the giant star is smaller than previously thought, making it much more difficult to explain how the red giant lost matter to its companion. The astronomers now think that, rather than streaming from one star to the other, the matter must be expelled from the giant star as a stellar wind and captured by the hotter companion.
“These observations have demonstrated the new snapshot imaging capability of the Very Large Telescope Interferometer. They pave the way for many further fascinating studies of interacting double stars,” concludes co-author Jean-Philippe Berger.
 The images were created from observations made with the Very Large Telescope Interferometer (VLTI) at ESOÊ¼s Paranal Observatory using the four 1.8-meter Auxiliary Telescopes to feed light into a new instrument called PIONIER (see ann11021).
PIONIER, developed at LAOG/IPAG in Grenoble, France, is a visiting instrument at the Paranal Observatory. PIONIER is funded by UniversitÃ© Joseph Fourier, IPAG, INSU-CNRS (ASHRA-PNPS-PNP) ANR 2G-VLTI and ANR Exozodi. IPAG is part of the Grenoble Observatory (OSUG).
The VLTI engineers had to control the distance traversed by the light from the widely separated telescopes with an accuracy of about one hundredth of the thickness of a strand of human hair. Once the light reached PIONIER, it was then channeled into the heart of the instrument: a remarkable optical circuit, smaller than a credit card, that finally brought the light waves from the different telescopes together in a very precise way so that they could interfere. The resulting resolving power of the telescope array has the sharpness not of the individual 1.8-meter Auxiliary Telescopes, but that of a much bigger “virtual telescope” about 130 meters across, limited only by how far apart the telescopes can be positioned.
The resolution of the NASA/ESA Hubble Space Telescope is approximately 50 milliarcseconds whereas the resolution attainable with the VLTI is about one milliarcsecond – corresponding to the apparent size of an astronaut on the surface of the Moon, seen from Earth.
This research was presented in a paper, “An incisive look at the symbiotic star SS Leporis – Milli-arcsecond imaging with PIONIER/VLTI”, by N. Blind et al. in press in the journal Astronomy & Astrophysics.
The team is composed of Nicolas Blind (UJF-Grenoble 1/CNRS-INSU, Institut de PlanÃ©tologie et d´Astrophysique de Grenoble, France [IPAG]), Henri Boffin (ESO, Chile), Jean-Philippe Berger (ESO, Chile), Jean-Baptiste Le Bouquin (IPAG, France), Antoine MÃ©rand (ESO, Chile), Bernard Lazareff (IPAG, France), and GÃ©rard Zins (IPAG, France).
ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organization in Europe and the world´s most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious program focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organizing cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world´s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world´s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 40-meter-class European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become “the world´s biggest eye on the sky”.
Image 1: These super-sharp images of the unusual vampire double star system SS Leporis were created from observations made with the VLT Interferometer at ESO´s Paranal Observatory using the PIONIER instrument. The system consists of a red giant star orbiting a hotter companion. The remarkable image sharpness – 50 times sharper than those from the NASA/ESA Hubble Space Telescope – not only allows the stars to be clearly separated and their orbital motion followed, but also allowed the size of the red giant to be measured more accurately than ever before. The system consists of a red giant star orbiting a hotter companion. Note that the stars have been artificially colored to match their known temperatures. Credit: ESO/PIONIER/IPAG
Image 2: This chart shows the location of the unusual double star system SS Leporis within the constellation of Lepus (The Hare). This map shows most of the stars visible to the unaided eye under good conditions and the star itself is marked within a red circle. This star is bright enough to be seen easily with the unaided eye on a clear night, not far from the familiar figure of Orion. Credit: ESO, IAU and Sky & Telescope
Image 3: This wide-field image of the sky around the unusual double star SS Leporis is a color composite made from exposures from the Digitized Sky Survey 2 (DSS2). The field of view is approximately 2.7 degrees. SS Leporis is the bright star at the center. The colored rings and the four spikes around the star are artifacts of the photographic process and the optics of the telescope used, and are not real. Credit: ESO/Digitized Sky Survey 2. Acknowledgment: Davide De Martin
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