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相关论文: Spitzer Surveys of IR Excesses of White Dwarfs

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IR excesses of white dwarfs (WDs) can be used to diagnose the presence of low-mass companions, planets, and circumstellar dust. Using different combinations of wavelengths and WD temperatures, circumstellar dust at different radial…

太阳与恒星天体物理 · 物理学 2015-05-20 Y. -H. Chu , R. A. Gruendl , J. Bilíkovà , A. Riddle , K. Y. -L. Su

Two types of dust disks around white dwarfs (WDs) have been reported: small dust disks around cool metal-rich WDs consisting of tidally disrupted asteroids, and a large dust disk around the hot central WD of the Helix planetary nebula (PN)…

In our Spitzer 24 \mu m survey of hot white dwarfs (WDs) and archival Spitzer study of pre-WDs, i.e., central stars of planetary nebulae (CSPNs), we found mid-IR excesses for -15 WDs/pre-WDs. These mid-IR excesses are indicative of the…

地球与行星天体物理 · 物理学 2015-03-18 J. Bilíkovà , Y. -H. Chu , K. Su , R. A. Gruendl , T. Rauch

We examine 14 hot white dwarfs for signs of infrared excess using the Spitzer Space Telescope. Twelve of the objects are massive white dwarfs which have been suggested to be the result of binary mergers. The remaining two objects are…

天体物理学 · 物理学 2008-11-26 Brad M. S. Hansen , Shri Kulkarni , Sloane Wiktorowicz

Infrared (IR) excess emission around white dwarfs (WDs) is commonly attributed to circumstellar debris disks and/or low-mass companions, providing a unique window into the evolution of planetary systems and binary evolution after the…

太阳与恒星天体物理 · 物理学 2026-04-14 Ke-Yi Wang , Qiong Liu

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,…

太阳与恒星天体物理 · 物理学 2015-06-04 Carolyn Brinkworth , Boris Gaensicke , Jon Girven , Don Hoard , Tom Marsh , Stephen Parsons , Detlev Koester

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…

地球与行星天体物理 · 物理学 2011-02-11 J. Farihi , M. Jura , B. Zuckerman

We report a Spitzer/IRAC search for infrared excesses around white dwarfs, including 14 newly-observed targets and 16 unpublished archived stars.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…

地球与行星天体物理 · 物理学 2015-05-30 S. Xu , M. Jura

Observations of atmospheric metals and dust discs around white dwarfs provide important clues to the fate of terrestrial planetary systems around intermediate mass stars. We present Spitzer IRAC observations of 15 metal polluted white…

地球与行星天体物理 · 物理学 2015-06-22 Carolina Bergfors , Jay Farihi , Patrick Dufour , Marco Rocchetto

White dwarfs whose atmospheres are polluted by terrestrial-like planetary debris have become a powerful and unique tool to study evolved planetary systems. This paper presents results for an unbiased Spitzer IRAC search for circumstellar…

地球与行星天体物理 · 物理学 2015-03-20 M. Rocchetto , J. Farihi , B. T. Gaensicke , C. Bergfors

Using the SDSS DR7 spectroscopic catalog, we searched the WISE AllWISE catalog to investigate the occurrence of warm dust, as inferred from IR excesses, around field M dwarfs (dMs). We developed SDSS/WISE color selection criteria to…

太阳与恒星天体物理 · 物理学 2015-04-14 Christopher A. Theissen , Andrew A. West

We describe a search for infra-red excess emission from dusty circumstellar material around 180,000 stars observed by the Kepler and WISE missions. This study is motivated by i) the potential to find bright warm disks around planet host…

地球与行星天体物理 · 物理学 2013-11-07 G. M. Kennedy , M. C. Wyatt

Circumstellar debris disks are important because of their connection to planetary systems. An efficient way to identify these systems is through their infrared excess. Most studies so far concentrated on early-type or solar-type stars, but…

太阳与恒星天体物理 · 物理学 2015-06-11 Henning Avenhaus , Hans Martin Schmid , Michael R. Meyer

Infrared excess is an important probe of sub-stellar companions and/or debris disks around white dwarfs (WDs). Such systems are still rare for in-depth understanding of their formation and long-term evolution. One of the largest…

太阳与恒星天体物理 · 物理学 2023-02-15 Lin Wang , Xiaoxia Zhang , Junfeng Wang , Zhi-Xiang Zhang , Taotao Fang , Wei-Min Gu , Jincheng Guo , Xiaochuan Jiang

Infrared excesses around white dwarf stars indicate the presence of various astrophysical objects of interest, including companions and debris disks. In this second paper of a series, we present follow-up observations of infrared excess…

In recent years, the number of white dwarfs (WDs) showing infrared (IR) excesses, attributed to circumstellar dust disks, has grown significantly. Gaseous disks have also been detected in some WDs with dust. We obtained optical spectra with…

太阳与恒星天体物理 · 物理学 2025-09-08 L. Saker , M. Gomez , L. Garcia

Spitzer Space Telescope IRAC 3-8 micron and AKARI IRC 2-4 micron photometry are reported for ten white dwarfs with photospheric heavy elements; nine relatively cool stars with photospheric calcium, and one hotter star with a peculiar high…

地球与行星天体物理 · 物理学 2015-03-13 J. Farihi , M. Jura , J. -E. Lee , B. Zuckerman

We have carried out $JHK_s$ imaging of 12 white dwarf debris disk candidates from the WIRED SDSS DR7 catalog, aiming to confirm or rule out disks among these sources. On the basis of positional identification and the flux density spectra,…

太阳与恒星天体物理 · 物理学 2015-06-16 Zhongxiang Wang , Anestis Tziamtzis , Xuebing Wang

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…

地球与行星天体物理 · 物理学 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 have identified four circumstellar disks with a deficit of dust emission from their inner 15-50 AU. All four stars have F-G spectral type, and were uncovered as part of the Spitzer Space Telescope ``Cores to Disks'' Legacy Program…

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