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Related papers: Metal-rich debris discs around white dwarfs

200 papers

We report Spitzer Space Telescope photometry of eleven externally-polluted white dwarfs. Of the nine stars for which we have IRAC photometry, we find that GD 40, GD 133 and PG 1015+161 each has an infrared excess that can be understood as…

Astrophysics · Physics 2009-06-23 M. Jura , J. Farihi , B. Zuckerman

Spitzer Space Observatory IRAC and MIPS photometric observations are presented for 20 white dwarfs with T < 20,000 K and metal-contaminated photospheres. A warm circumstellar disk is detected at GD 16 and likely at PG 1457-086, while the…

Earth and Planetary Astrophysics · Physics 2011-02-11 J. Farihi , M. Jura , B. Zuckerman

SDSS J030308.35+005444.1 is a close, detached, eclipsing white dwarf plus M dwarf binary which shows a large infrared excess which has been interpreted in terms of a circumbinary dust disk. In this paper we present optical and near-infrared…

Solar and Stellar Astrophysics · Physics 2015-06-16 S. G. Parsons , T. R. Marsh , B. T. Gänsicke , M. R. Schreiber , M. C. P. Bours , V. S. Dhillon , S. P. Littlefair

We present Spitzer Space Telescope data of four isolated white dwarfs that were previously known to harbor circumstellar gaseous disks. IRAC photometry shows a significant infrared excess in all of the systems, SDSS0738+1835, SDSS0845+2257,…

Solar and Stellar Astrophysics · Physics 2015-06-04 Carolyn Brinkworth , Boris Gaensicke , Jon Girven , Don Hoard , Tom Marsh , Stephen Parsons , Detlev Koester

We identify SDSSJ121010.1+334722.9 as an eclipsing post-common-envelope binary, with an orbital period of P ~ 3 hrs, containing a very cool, low-mass, DAZ white dwarf and a low-mass main-sequence star of spectral type M5. A model atmosphere…

Spectroscopic observations of white dwarfs reveal that many of them are polluted by exoplanetary material, whose bulk composition can be uniquely probed this way. We present a spectroscopic and photometric analysis of the DA white dwarf…

The presence of planetary material in white dwarf atmospheres, thought to be accreted from a dusty debris disc produced via the tidal disruption of a planetesimal, is common. Approximately five per cent of these discs host a co-orbital…

Cool white dwarf stars are usually found to have an outer atmosphere that is practically pure in hydrogen or helium. However, a small fraction have traces of heavy elements that must originate from the accretion of extrinsic material, most…

Solar and Stellar Astrophysics · Physics 2015-05-19 P. Dufour , M. Kilic , G. Fontaine , P. Bergeron , F. -R. Lachapelle , S. J. Kleinman , S. K. Leggett

We present follow-up photometry and spectroscopy of ZTF J0328$-$1219 strengthening its status as a white dwarf exhibiting transiting planetary debris. Using TESS and Zwicky Transient Facility photometry, along with follow-up high speed…

This letter reports the first JWST spectroscopy of a white dwarf debris disk, giving a preliminary assessment of the salient features, and recommendations for future observations. The polluted and dusty star WD 0145+234 experienced a major…

Earth and Planetary Astrophysics · Physics 2023-12-21 Andrew Swan , Jay Farihi , Kate Y. L. Su , Steven J. Desch

WD J204713.76-125908.9 is a new addition to the small class of white dwarfs with helium-dominated photospheres that exhibit strong Balmer absorption lines and atmospheric metal pollution. The exceptional abundances of hydrogen observed in…

The detection of a dust disc around G29-38 and transits from debris orbiting WD1145+017 confirmed that the photospheric trace metals found in many white dwarfs arise from the accretion of tidally disrupted planetesimals. The composition of…

We have performed a comprehensive ground-based observational program aimed at characterizing the circumstellar material orbiting three single white dwarf stars previously known to possess gaseous disks. Near-infrared imaging unambiguously…

Solar and Stellar Astrophysics · Physics 2015-05-19 C. Melis , M. Jura , L. Albert , B. Klein , B. Zuckerman

We present VLT spectroscopy and NTT photometry of the faint cataclysmic binary SDSS J003941.06+005427.5. This object shows triple-peaked H-alpha emission with all three peaks variable in both strength and velocity. We measure an orbital…

Solar and Stellar Astrophysics · Physics 2015-05-20 John Southworth , T. R. Marsh , B. T. Gansicke , D. Steeghs , C. M. Copperwheat

For a fraction of single white dwarfs with debris disks, an additional gaseous disk was discovered. Both dust and gas are thought to be created by the disruption of planetary bodies. The composition of the extrasolar planetary material can…

Solar and Stellar Astrophysics · Physics 2014-11-11 S. Hartmann , T. Nagel , T. Rauch , K. Werner

Debris disk detections around M dwarfs are rare, and so far no gas emission has been detected from an M dwarf debris disk. This makes the 45 Myr old M dwarf WISEJ080822.18-644357.3 a bit of a curiosity; it has a strong infrared excess at an…

Solar and Stellar Astrophysics · Physics 2019-02-20 Kevin M. Flaherty , A. Meredith Hughes , Eric E. Mamajek , Simon J. Murphy

Numerous white dwarf stars are known to be orbited by disks of gas and dust. To date, broad, about 300 km s-1 wide, gaseous circumstellar absorption features have only been reported for the already iconic WD 1145+017, where one is…

This letter reports 12 novel spectroscopic detections of warm circumstellar dust orbiting polluted white dwarfs using JWST MIRI. The disks span two orders of magnitude in fractional infrared brightness and more than double the number of…

Earth and Planetary Astrophysics · Physics 2025-01-31 J. Farihi , K. Y. L. Su , C. Melis , S. J. Kenyon , A. Swan , S. Redfield , M. C. Wyatt , J. H. Debes

We report a Spitzer/IRAC search for infrared excesses around white dwarfs, including 14 newly-observed targets and 16 unpublished archived stars. We find a substantial infrared excess around two warm white dwarfs --- J220934.84+122336.5 and…

Earth and Planetary Astrophysics · Physics 2015-05-30 S. Xu , M. Jura

We report on our attempt for the first non-LTE modeling of gaseous metal disks around single DAZ white dwarfs recently discovered by Gaensicke et al. and thought to originate from a disrupted asteroid. We assume a Keplerian rotating viscous…

Astrophysics · Physics 2009-07-22 K. Werner , T. Nagel , T. Rauch