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We review the nearby debris disk structures revealed by multi-wavelength images from Spitzer and Herschel, and complemented with detailed spectral energy distribution modeling. Similar to the definition of habitable zones around stars,…

地球与行星天体物理 · 物理学 2015-06-16 Kate Y. L. Su , George H. Rieke

Although photometric and spectroscopic surveys with the Spitzer Space Telescope increased remarkably the number of well studied debris disks around A-type and Sun-like stars, detailed analyzes of debris disks around F-type stars remained…

太阳与恒星天体物理 · 物理学 2015-05-20 A. Moór , I. Pascucci , Á. Kóspál , P. Ábrahám , T. Csengeri , L. L. Kiss , D. Apai , C. Grady , Th. Henning , Cs. Kiss , D. Bayliss , A. Juhász , J. Kovács , T. Szalai

We present near-infrared spectroscopic observations of 20 previously known DAZ white dwarfs obtained at the NASA Infrared Telescope Facility. Two of these white dwarfs (G29-38 and GD362) are known to display significant K-band excesses due…

天体物理学 · 物理学 2009-11-11 Mukremin Kilic , Ted von Hippel , S. K. Leggett , D. E. Winget

We present an analysis of the near-infrared continuum emission from the circumstellar gas disks of Be stars using a radiative transfer code for a parametrized version of the viscous decretion disk model. This isothermal gas model creates…

太阳与恒星天体物理 · 物理学 2015-05-27 Y. Touhami , D. R. Gies , G. H. Schaefer

The $Herschel$ Space telescope carried out an unprecedented survey of nearby stars for debris disks. The dust present in these debris disks scatters and polarizes stellar light in the visible part of the spectrum. We explore what can be…

地球与行星天体物理 · 物理学 2019-02-12 Julien Vandeportal , Pierre Bastien , Amélie Simon , Jean-Charles Augereau , Émilie Storer

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

We present a Spitzer MIPS study of the decay of debris disk excesses at 24 and 70 $\mu$m for 255 stars of types F4 - K2. We have used multiple tests, including consistency between chromospheric and X-ray activity and placement on the HR…

地球与行星天体物理 · 物理学 2015-06-18 J. M. Sierchio , G. H. Rieke , K. Y. L. Su , Andras Gaspar

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…

太阳与恒星天体物理 · 物理学 2015-05-19 C. Melis , M. Jura , L. Albert , B. Klein , B. Zuckerman

Debris disks or exo-Kuiper belts, detected through their thermal or scattered emission from their dusty components, are ubiquitous around main-sequence stars. Since dust grains are short-lived, their sustained presence is thought to require…

地球与行星天体物理 · 物理学 2024-03-18 Antranik A. Sefilian

High-precision interferometric observations of six early-type main sequence stars known to harbour cold debris discs have been obtained in the near-infrared K band with the FLUOR instrument at the CHARA Array. The measured squared…

We present an analysis on the potential prevalence of mid infrared excesses in stars with and without planetary companions. Based on an extended database of stars detected with the ${\it WISE}$ satellite, we studied two stellar samples: one…

太阳与恒星天体物理 · 物理学 2017-08-23 Raul F. Maldonado , Miguel Chavez , Emanuele Bertone , Fernando Cruz-Saenz de Miera

The $\textit{Herschel}$ DEBRIS, DUNES and GT programmes observed 37 exoplanet host stars within 25 pc at 70, 100 and 160 $\mu$m with the sensitivity to detect far-infrared excess emission at flux density levels only an order of magnitude…

Using data from the WISE All-Sky Survey, we have found >100 new infrared excess sources around main-sequence Hipparcos stars within 75pc. Our empirical calibration of WISE photospheric colors and removal of non-trivial false-positive…

太阳与恒星天体物理 · 物理学 2016-02-03 Rahul Patel , Stanimir Metchev , Aren Heinze , Joseph Trollo

Multi-epoch infrared photometry from Spitzer is used to monitor circumstellar discs at white dwarfs, which are consistent with disrupted minor planets whose debris is accreted and chemically reflected by their host stars. Widespread…

太阳与恒星天体物理 · 物理学 2020-07-29 Andrew Swan , Jay Farihi , Thomas G. Wilson , Steven G. Parsons

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 present our first results from a high-contrast imaging search for planetary mass companions around stars with gapped debris disks, as inferred from the stars' bright infrared excesses. For the six considered stars, we model the disks'…

地球与行星天体物理 · 物理学 2015-06-23 Tiffany Meshkat , Vanessa P. Bailey , Kate Y. L. Su , Matthew A. Kenworthy , Eric E. Mamajek , Philip M. Hinz , Paul S. Smith

We present the first characterisation of the 12um warm dust ("exo-Zodi") luminosity function around Sun-like stars, focussing on the dustiest systems that can be identified by WISE. We detect six new warm dust candidates, five of which have…

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

We report the results of a ${\sim}4$-year direct imaging survey of 104 stars to resolve and characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager Exoplanet Survey. We targeted nearby (${\lesssim}150$…

We assess the current membership of the nearby, young TW Hydrae Association and examine newly proposed members with the Wide-field Infrared Survey Explorer (WISE) to search for infrared excess indicative of circumstellar disks. Newly…

太阳与恒星天体物理 · 物理学 2015-06-05 Adam Schneider , Carl Melis , Inseok Song

Unlike hot Jupiters or other gas giants, super-Earths are expected to have a wide variety of compositions, ranging from terrestrial bodies like our own to more gaseous planets like Neptune. Observations of transiting systems, which allow us…