≡ Menu

Focus on Massive Stars

Pismis 24 clusterWhat got me interested in Pismis 24-1 was simply the image. It’s one of those spectacular displays we’ve come to expect from Hubble, obtained using the telescope’s Advanced Camera for Surveys. Pismis 24-1 is part of the open cluster Pismis 24, some 8000 light years from Earth in the nebula NGC 6357 in Sagittarius. The cluster is filled with massive stars, but what seizes the attention is the juxtaposition of the cluster itself (the brightest stars in the image) and the gorgeous tapestries of the nebula in which it is embedded.

Pismis 24-1, the brightest star in the cluster, was originally thought to weigh up to 300 solar masses, making it twice the assumed upper mass limit for individual stars. But as the image below shows, it’s at least a binary, and ground based observations suggest that it may even be a triple system, with the third star too tightly bound to be resolved. If so, it’s a whopper of one, each of the three stars averaging about 70 solar masses. Ahead for these behemoths is a short lifetime of a few million years and a violent end as a supernova before the inevitable collapse into a black hole.

Pismis 24-1 resolvedHow unusual is this configuration? According to a Hubble news release, there are 18,000 solar-mass stars for every star with 65 solar masses or more. But the numbers are deceptive, since stars like our Sun live 3,000 times longer than their giant counterparts. So the galaxy today holds millions of solar-mass stars for each of its vast cousins. This work, conducted by Jesús Maíz Apellániz (Instituto de Astrofísica de Andalucía) should be useful as we firm up our knowledge of the conditions leading to supernova explosions, those titanic events that seed the universe with heavy elements.

Image credits: Credit: NASA, ESA, and J. Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain).

Comments on this entry are closed.

  • ljk February 5, 2008, 10:38

    A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernovae

    Authors: C.S. Kochanek (1,3), J.F. Beacom (1,2,3), M.D. Kistler (2,3), J.L. Prieto (1,3) K.Z. Stanek (1,3), T.A. Thompson (1,3), H. Yuksel (2,3) ((1) Department of Astronomy, The Ohio State University, (2) Department of Physics, The Ohio State University, (3) Center for Cosmology and Astroparticle Physics, The Ohio State University)

    (Submitted on 4 Feb 2008)

    Abstract: Extragalactic transient searches have historically been limited to looking for the appearance of new sources such as supernovae. We propose a new kind of survey that will do the opposite, that is, search for the disappearance of massive stars. This will entail the systematic observation of galaxies within a distance of 10 Mpc in order to watch ~1 million supergiants. Reaching this critical number ensures that we will see something occur yearly, since these massive stars must end their lives with a core collapse within ~1 million years.

    Using deep imaging and image subtraction it is possible to determine the fates of these stars whether they end with a bang (supernova) or a whimper (fall out of sight). Such a survey would place completely new limits on the total rate of all core collapses, which is critical for determining the validity of supernova models. The designed sensitivity of such a survey will also allow us determine the properties of supernova progenitors, better characterize poorly understood optical transients, such as eta Carina-like mass ejections, find and characterize large numbers of Cepheids, luminous blue variables and eclipsing binaries, and allow the discovery of any new phenomena which inhabit this relatively unexplored parameter space.

    Comments: 6 pages, 3 figures, submitted to ApJ

    Subjects: Astrophysics (astro-ph)

    Cite as: arXiv:0802.0456v1 [astro-ph]

    Submission history

    From: Christopher S. Kochanek [view email]

    [v1] Mon, 4 Feb 2008 17:09:48 GMT (37kb)

    http://arxiv.org/abs/0802.0456