Showing posts with label M4. Show all posts
Showing posts with label M4. Show all posts

Monday, June 13, 2016

Asteroseismologists listen to the relics of the Milky Way: sounds from the oldest stars in our Galaxy

An image of the globular star cluster M4, made with the MPG/ESO 2.2-m telescope at the La Silla Observatory in Chile. The yellow circles mark the positions of the stars observed in the new study. Click the image for an animation and audio from each star. Credit: ESO / University of Birmingham. Hi-res image


Astrophysicists from the University of Birmingham have captured the sounds of some of the oldest stars in our galaxy, the Milky Way, according to research published today in thejournal Monthly Notices of the Royal Astronomical Society.

The research team, from the University of Birmingham's School of Physics and Astronomy, has reported the detection of resonant acoustic oscillations of stars in 'M4', one of the oldest known clusters of stars in the Galaxy, some 13 billion years old.

Using data from the NASA Kepler/K2 mission, the team has studied the resonant oscillations of stars using a technique called asteroseismology. These oscillations lead to miniscule changes or pulses in brightness, and are caused by sound trapped inside the stars. By measuring the tones in this 'stellar music', it is possible to determine the mass and age of individual stars. (You can listen to the sound of each star here.)

This discovery opens the door to using asteroseismology to study the very early history of our Galaxy.

Dr Andrea Miglio, from the University of Birmingham's School of Physics and Astronomy, who led the study, said: 'We were thrilled to be able to listen to some of the stellar relics of the early universe. The stars we have studied really are living fossils from the time of the formation of our Galaxy, and we now hope be able to unlock the secrets of how spiral galaxies, like our own, formed and evolved.'

Dr Guy Davies, from the University of Birmingham's School of Physics and Astronomy, and co-author on the study, said: 'The age scale of stars has so far been restricted to relatively young stars, limiting our ability to probe the early history of our Galaxy. In this research we have been able to prove that asteroseismology can give precise and accurate ages for the oldest stars in the Galaxy '

Professor Bill Chaplin, from the University of Birmingham's School of Physics and Astronomy and leader of the international collaboration on asteroseismology, said: 'Just as archaeologists can reveal the past by excavating the earth, so we can use sound inside the stars to perform Galactic archaeology.'



Further information

The new work appears in "Detection of solar-like oscillations in relics of the Milky Way: asteroseismology of K giants in M4 using data from the NASA K2 mission", A. Miglio, W. J. Chaplin, K. Brogaard, M. N. Lund, B. Mosser, G. R. Davies, R. Handberg, A. P. Milone, A. F. Marino, D. Bossini, Y. P. Elsworth, F. Grundahl, T. Arentoft, L. R. Bedin, T. L. Campante, J. Jessen-Hansen, C. D. Jones, J. S. Kuszlewicz, L. Malavolta, V. Nascimbeni and E. L. Sandquist, Monthly Notices of the Royal Astronomical Society, in press.



Media contact

Harrison
Media Relations Manager
University of Birmingham
Tel: +44 (0)121 414 5134
Mob: +44 (0)7789 921163

l.harrison.1@bham.ac.uk



Science contact

Prof Andrea Miglio
University of Birmingham

miglioa@bison.ph.bham.ac.uk
 


Notes for editors

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Wednesday, July 30, 2014

Binary Stars in the Globular Cluster Messier 4

An image of the globular cluster Messier 4
New observations of M4 have studied the binary stars in this cluster.
Credit: ESO

A globular cluster is a roughly spherical ensemble of stars, as many as several million of them, gravitationally bound together in groups whose diameters can be as small as only tens of light-years. To sense the dramatic implications of this dense packing, consider that the nearest star to the Sun, Proxima Centauri, is about four light-years away. Messier 4 (M4) is the closest globular cluster to Earth at a distance of about six thousand light-years, and a puzzle to astronomers. Normal gravitational effects should, over time, redistribute the stars in a globular cluster until they are more numerous towards the center, but while M4 shows a central concentration of stars it does not show evidence for a steep central cusp even though astronomers think enough time has passed.

To understand what is going on in this globular cluster, and to help understand how these clusters evolve in general, CfA astronomer Maureen van den Berg and her collaborators have undertaken a large and unprecedented set of deep images of M4 with the Hubble Space Telescope to look for binary stars, that is stars with companions. The dynamical interactions between the densely crowded stars in a globular cluster should disrupt many such binaries, but for reasons that are not understood about fifteen percent of the stars in M4 are binaries, at least based on monitoring brightness variations (a more typical number is two percent). Whether or not this unusual abundance is connected to the lack of a central cusp in stellar density is also not understood.

The astronomers set out to use Hubble to study the binary star population in M4 looking at both brightness variations and stellar wobble (astrometric) variations, in particular due to binaries with a massive, faint, and evolved companion like a white dwarf or neutron star. The team was able to find and characterize a much more complete set of binaries, including thirty-six new variables. They note in passing that, as part of the search process, any stars with massive "hot Jupiter" exoplanet companions would probably also have been detected, but that none were. The extensive results are still being analyzed, but the improved statistics will make the conclusions much more reliable.

Reference(s):
 
"The M 4 Core Project with HST – III. Search for Variable Stars in the Primary Field," V. Nascimbeni, L. R. Bedin, D. C. Heggie, M. van den Berg, M. Giersz, G. Piotto, K. Brogaard, A. Bellini, A. P. Milone, R. M. Rich, D. Pooley, J. Anderson,, L. Ubeda, S. Ortolani, L. Malavolta, A. Cunial1, and A. Pietrinferni, MNRAS 442, 2381, 2014