FIRST DETECTION OF KRYPTON AND XENON IN A WHITE DWARF

Journal Article · Sun Jul 01 00:00:00 EDT 2012 · Astrophysical Journal Letters

DOI:https://doi.org/10.1088/2041-8205/753/1/L7· OSTI ID:22047717

Werner, Klaus; Rauch, Thomas; Ringat, Ellen ^[1]; Kruk, Jeffrey W ^[2]

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1. Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University Tuebingen, Sand 1, 72076 Tuebingen (Germany)
2. NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)

We report on the first detection of the noble gases krypton (Z = 36) and xenon (54) in a white dwarf. About 20 Kr VI- VII and Xe VI- VII lines were discovered in the ultraviolet spectrum of the hot DO-type white dwarf RE 0503-289. The observations, performed with the Far Ultraviolet Spectroscopic Explorer, also reveal highly ionized photospheric lines from other trans-iron group elements, namely Ga (31), Ge (32), As (33), Se (34), Mo (42), Sn (50), Te (52), and I (53), from which gallium and molybdenum are new discoveries in white dwarfs, too. For Kr and Xe, we performed an NLTE analysis and derived mass fractions of log Kr = -4.3 {+-} 0.5 and log Xe = -4.2 {+-} 0.6, corresponding to an enrichment by factors of 450 and 3800, respectively, relative to the Sun. The origin of the large overabundances is unclear. We discuss the roles of neutron-capture nucleosynthesis in the precursor star and radiation-driven diffusion. It is possible that diffusion is insignificant and that the observed metal abundances constrain the evolutionary history of the star. Its hydrogen deficiency may be the consequence of a late helium-shell flash or a binary white dwarf merger.

• OSTI ID: 22047717
• Journal Information: Astrophysical Journal Letters, Vol. 753, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 2041-8205
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ASTROPHYSICS
BINARY STARS
CAPTURE
DIFFUSION
ELEMENT ABUNDANCE
FAR ULTRAVIOLET RADIATION
GALLIUM
HELIUM
HYDROGEN
IRON
KRYPTON
MOLYBDENUM
NEUTRON REACTIONS
NUCLEOSYNTHESIS
PHOTOSPHERE
ULTRAVIOLET SPECTRA
WHITE DWARF STARS
XENON