Unusual Massive White Dwarf Stars Have Oxygen Atmospheres
Written by Nancy Atkinson
White dwarfs are strange stars, but researchers recently discovered two of the strangest yet. However, these two oddballs are a missing link of sorts, between massive stars that end their lives as supernovae and small to medium sized stars that become white dwarfs. Somehow, these two once-massive stars avoided the core collapse of a supernova, and are the only two white dwarfs known to have oxygen-rich atmospheres. These so-called massive white dwarfs have been predicted, but never before observed.
The stars, named SDSS 0922+2928 and SDSS 1102+2054 are 400 and 220 light years from Earth. They are both remnants of massive stars that are at the end of their stellar evolution having consumed all the material they had available for nuclear fusion.
The low levels of carbon visible in their spectra indicate the stars have shed part of their outer layers and burned the carbon contained in their cores.
"These surface abundances of oxygen imply that these are white dwarfs displaying their bare oxygen-neon cores, and that they may have descended from the most massive progenitors stars in that class," said astrophysicist Dr. Boris Gänsicke from the University of Warwick, lead author on a paper appearing in this week's edition of Science Express.
Dr. Boris Gänsicke from the department of physics at the University of Warwick.
Gänsicke told Universe Today that he and his team didn't start out specifically looking for these previously theoretical stars. "I've been working with our research student Jonathan Girven on several projects on white dwarfs, and we came across a range of unusual looking objects — some we are still puzzling what they are. From a theoretical perspective, I was wondering if white dwarfs with oxygen-rich atmospheres exist, and combining both angles, we developed a specific search for these stars."
In a search of Sloan Digital Sky Survey data, the astrophysicists did indeed discover two white dwarfs with large atmospheric oxygen abundances.
Almost all white dwarfs have hydrogen and/or helium envelopes that, while low in mass, are sufficiently thick to shield the core from direct view. Theoretical models predicted that if stars around 7 – 10 times the mass of our own Sun don't end their lives as supernovae, the other option is that they will consume all of their hydrogen, helium and carbon, and end their lives as white dwarfs with very oxygen-rich cores.
Astrophysicists could then detect an extremely oxygen-rich spectrum from the surface of the white dwarf.
Most stellar models producing white dwarfs with such oxygen and neon cores also predict that a sufficiently thick carbon-rich layer should surround the core and avoid upward diffusion of large amounts of oxygen.
However, calculations also show that the thickness of this layer decreases the closer the progenitor star is to upper mass limit for stars ending their lives as white dwarfs. Hence one possibility for the formation of SDSS 0922+2928 and SDSS 1102+2054 is that they descended from the most massive stars avoiding core-collapse, in which case they would be expected to be very massive themselves. However current data is insufficient to provide any unambiguous measure of the masses of these two unusual stars.
What is the future for these massive white dwarfs? Gänsicke said the two stars will evolve very slowly. "Given that they are burnt-out stellar cores that do no longer undergo nuclear fusion, their destiny is to continue cooling and fading. This will be a very slow process, and any noticeable change in their appearance will take 10s to 100s million years."
Lead image caption: Sloan Digital Sky Survey spectroscopy of this inconspicuous blue object — SDSS1102+2054 — reveals it to be an extremely rare stellar remnant: a white dwarf with an oxygen-rich atmosphere
Sources: Science, email interview with Gänsicke
Filed under: Astronomy
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November 12th, 2009 at 5:48 pm
What surface temperatures are we looking at in these massive oxygen/neon-rich white dwarfs?
November 12th, 2009 at 7:24 pm
Just posted at the arXiv site: http://arxiv.org/PS_cache/arxiv/pdf/0911/0911.2246v1.pdf . Haven't had time to closely read, but enjoy
November 12th, 2009 at 7:46 pm
Looks like surface temps of 8000-9000K seem to best fit massive WD models.
November 13th, 2009 at 1:21 am
The theoretical nature of WD stars is best viewed in the graphic "Nature of Compact Remnants"
The life and times of an intermediate mass star – In isolation/in a close binary by Ivan Iben Jr. (1985) [QJRAS., 26, 11, pg.31 (1995)]
Such stars can be anywhere between 1.4 and 1.1 Solar Masses, whose original progenitor mass is between 8 and 10 solar masses.
I'm certain other oxygen WD's have been observed and catalogued, so I don't think this is the first time they have been found – in isolation or in binary stars. (Have to look for them though.)
Red giant stars on the H-R Diagrams that for these kind of systems are called super-AGB stars (AGB- Asymptotic Giant Stars)
November 13th, 2009 at 1:25 am
Yeah, I though so…
Oxygen WD examples include;
GD984, REJ1032+532, and REJ2156-543
I.e. Probing the Atmospheres of Hot DA White Dwarfs with O VI
Chayer, P.ASPC., 348, 209 (2006)
There are others…
November 13th, 2009 at 6:03 am
It is interesting he appears to have done this work with a modest telescope.
I suppose this makes sense, where neutron stars have an iron surface, most white dwarf stars have helium carbon surface or atmospheres, so in between are these oxygen neon objects.
LC
November 13th, 2009 at 7:02 am
Thanks for those links, HSBC, on oxygen dominated white dwarfs. I remember seeing some work on these WDs over the past decade. The authors of the current paper state "The only plausible explanation for the observed O/C abundances is that these two WDs have overall very low carbon mass fractions, and hence represent naked ONe cores. As such, they are distinct from 1H1504+65 and the "hot" DQ white dwarfs."
While noting that their current data is insufficient to accurately determine the masses of these objects, the authors do posit that their progenitors may have descended from the most massive stars avoiding core collapse, in which case these WDs would be expected to be massive too.
November 13th, 2009 at 6:33 pm
Don't know if this is allowed but, in case you haven't gone back to the "Great Observatories Combine…." thread, I'll offer my thanks here for that great link you provided me. It was "most" informative. Damn this is fun.
November 13th, 2009 at 6:34 pm
Sorry, that was for you Jon.
November 13th, 2009 at 7:47 pm
While comment awaits moderation,
@wjwbudro, I've since had the time to read the paper on Hubble's Paschen-alpha mosaic and I'm just floored. I'm surprised the Hubble site didn't present some of the close-ups of the galactic center reproduced in the paper. The Arches Cluster, Pistol Star, Sgr- A* region, faint filaments and numerous Pa-alpha point sources. This paper has a little something for everyone. (Btw, the hi-res version of this paper is available at: http://arxiv.org/abs/0911.2226 ). Glad you got to take a look at this phenomenal mosaic
November 13th, 2009 at 7:50 pm
Fertile hunting ground for current or future astronomical press releases can be found browsing at the arXiv pre-print server M-F ( http://arxiv.org/list/astro-ph/new ), plus a slew of papers covering many (unreported) facets of modern astronomy.
November 13th, 2009 at 8:57 pm
I copied the near infrared image to Win pic/fax viewer to zoom in. Our BH is alive and hungry. Sorry folks but, this is exciting stuff.
http://hubblesite.org/newscenter/archive/releases/2009/28/image/
November 14th, 2009 at 6:13 am
These are stunning images. The transitions from n = 3 to n' > 3 levels, the Paschen series in the H-spectrum is in the infrared region. Some of this has been done with the Spitzer, as indicated in the mozaic.
I am not sure what bearing this has on O-containing white dwarfs, but this is an interesting diversion.
LC