eso1326 — Science Release

New Kind of Variable Star Discovered

Minute variations in brightness reveal whole new class of stars

12 June 2013

Astronomers using the Swiss 1.2-metre Euler telescope at ESOòÀÙs La Silla Observatory in Chile have found a new type of variable star. The discovery was based on the detection of very tiny changes in brightness of stars in a cluster. The observations revealed previously unknown properties of these stars that defy current theories and raise questions about the origin of the variations.

The Swiss are justly famed for their craftsmanship when creating extremely precise pieces of technology. Now a Swiss team from the Geneva Observatory has achieved extraordinary precision using a comparatively small 1.2-metre telescope for an observing programme stretching over many years. They have discovered a new class of variable stars by measuring minute variations in stellar brightness.

The new results are based on regular measurements of the brightness of more than three thousand stars in the open star cluster NGC 3766 [1] over a period of seven years. They reveal how 36 of the clusteròÀÙs stars followed an unexpected pattern òÀÔ they had tiny regular variations in their brightness at the level of 0.1% of the starsòÀÙ normal brightness. These variations had periods between about two and 20 hours. The stars are somewhat hotter and brighter than the Sun, but otherwise apparently unremarkable. The new class of variable stars is yet to be given a name.

This level of precision in the measurements is twice as good as that achieved by comparable studies from other telescopes òÀÔ and sufficient to reveal these tiny variations for the first time.

òÀÜWe have reached this level of sensitivity thanks to the high quality of the observations, combined with a very careful analysis of the data,òÀÝ says Nami Mowlavi, leader of the research team, òÀÜbut also because we have carried out an extensive observation programme that lasted for seven years. It probably wouldnòÀÙt have been possible to get so much observing time on a bigger telescope.òÀÝ

Many stars are known as variable or pulsating stars, because their apparent brightness changes over time. How the brightness of these stars changes depends in complex ways on the properties of their interiors. This phenomenon has allowed the development of a whole branch of astrophysics called asteroseismology, where astronomers can òÀÜlistenòÀÝ to these stellar vibrations, in order to probe the physical properties of the stars and get to know more about their inner workings.

òÀÜThe very existence of this new class of variable stars is a challenge to astrophysicists,òÀÝ says Sophie Saesen, another team member. òÀÜCurrent theoretical models predict that their light is not supposed to vary periodically at all, so our current efforts are focused on finding out more about the behaviour of this strange new type of star.òÀÝ

Although the cause of the variability remains unknown, there is a tantalising clue: some of the stars seem to be fast rotators. They spin at speeds that are more than half of their critical velocity, which is the threshold where stars become unstable and throw off material into space.

òÀÜIn those conditions, the fast spin will have an important impact on their internal properties, but we are not able yet to adequately model their light variations,òÀÝ explains Mowlavi. òÀÜWe hope our discovery will encourage specialists to address the issue in the hope of understanding the origin of these mysterious variations.òÀÝ

Notes

[1] This star cluster is one of several included in this major monitoring programme. NGC 3766 lies about 7000 light-years from Earth in the southern constellation of Centaurus (The Centaur) and is estimated to be about 20 million years old.

More information

This research was presented in a paper òÀÜStellar variability in open clusters I. A new class of variable stars in NGC 3766òÀÝ, by N. Mowlavi et al., published in the journal Astronomy & Astrophysics on 12 June 2013.

The team is composed of N. Mowlavi, F. Barblan, S. Saesen and L. Eyer. All four authors are from the Geneva Observatory in Switzerland.

ESO is the foremost intergovernmental astronomy organisation in Europe and the worldòÀÙs most productive ground-based astronomical observatory by far. 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 programme 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 organising 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 worldòÀÙs most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the worldòÀÙs 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 the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become òÀÜthe worldòÀÙs biggest eye on the skyòÀÝ.

Links

• Research paperˆà
• More information about the Swiss 1.2-metre Leonhard Euler Telescope

Contacts

Nami Mowlavi
Geneva Observatory, University of Geneva/ISDC
Switzerland
Tel: +41 22 37 92 194
Email: Nami.Mowlavi@unige.ch

Sophie Saesen
Geneva Observatory, University of Geneva
Switzerland
Tel: +41 22 379 24 46
Email: Sophie.Saesen@unige.ch

Richard Hook
ESO Public Information Officer
Garching bei M†®nchen, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591
Email: rhook@eso.org

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