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相关论文: Faint warm debris disks around nearby bright stars…

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Circumstellar dust disks have been observed around many nearby stars. However, many stars are part of binary or multiple stellar systems. A natural question arises regarding the presence and properties of such disks in systems with more…

太阳与恒星天体物理 · 物理学 2019-08-17 David R. Rodriguez , Gaspard Duchene , Henry Tom , Grant Kennedy , Brenda Matthews , Jane Greaves , Harold Butner

As part of a large Spitzer/MIPS GTO program, we have searched for infrared excesses due to debris disks toward 26 FGK field stars known from radial velocity (RV) studies to have one or more planets. While none of these stars show excesses…

We describe calculations for the formation of icy planets and debris disks at 30-150 AU around 1-3 solar mass stars. Debris disk formation coincides with the formation of planetary systems. As protoplanets grow, they stir leftover…

天体物理学 · 物理学 2009-11-13 Scott J. Kenyon , Benjamin C. Bromley

The Kepler Mission recently identified 997 systems hosting candidate extrasolar planets, many of which are super-Earths. Realizing these planetary systems are candidates to host extrasolar asteroid belts, we use mid-infrared data from the…

地球与行星天体物理 · 物理学 2015-06-03 S. M. Lawler , B. Gladman

We present a search for debris discs amongst M-dwarf members of nearby, young (5-150 Myr) moving groups (MGs) using infrared (IR) photometry, primarily from the Wide Infrared Survey Explorer (WISE). A catalogue of 100 MG M-dwarfs that have…

太阳与恒星天体物理 · 物理学 2017-05-31 Alex S. Binks , Robin D. Jeffries

We present the results of a Spitzer photometric investigation into the IR excesses of close binary systems. In a sample of 10 objects, excesses in IRAC and MIPS24 bands implying the presence of warm dust are found for 3. For 2 objects we do…

地球与行星天体物理 · 物理学 2015-05-19 M. Matranga , J. J. Drake , V. L. Kashyap , M. Marengo , M. J. Kuchner

The presence of debris disks around $\sim$ 1-Gyr-old main sequence stars suggests that an appreciable amount of dust may persist even in mature planetary systems. Here we report the detection of dust emission from 55 Cancri, a star with…

Debris disks are dusty, gas-poor disks around main sequence stars (Backman & Paresce 1993; Lagrange, Backman & Artymowicz 2000; Zuckerman 2001). Micron-sized dust grains are inferred to exist in these systems from measurements of their…

天体物理学 · 物理学 2007-05-23 Christine H. Chen

We use Spitzer Space Telescope 24 {\mu}m data to search for debris disks among 122 AFGKM stars from the \sim 670 Myr clusters Hyades, Coma Ber, and Praesepe, utilizing a number of advances in data reduction and determining the intrinsic…

星系天体物理 · 物理学 2012-04-24 Laurie Urban , George Rieke , Kate Su , David E. Trilling

Gas has been detected in a number of debris disk systems. This gas may have arisen from grain sublimation or grain photodesorption. It interacts with the surrounding dust grains through a number of charge and heat exchanges. Studying the…

地球与行星天体物理 · 物理学 2018-11-14 Kyryl Zagorovsky , Alexis Brandeker , Yanqin Wu

Observations of circumstellar disks provide a powerful tool for our understanding of planetary systems dynamics. Analogs to the Solar System asteroid belts, debris disks result from the collision of the remaining solid material of the…

Recent interferometric surveys of nearby main-sequence stars show a faint but significant near-infrared excess in roughly two dozen systems, i.$\,$e. around $10\,\%$ to $30\,\%$ of stars surveyed. This excess is attributed to dust located…

太阳与恒星天体物理 · 物理学 2017-02-01 Florian Kirchschlager , Sebastian Wolf , Alexander V. Krivov , Harald Mutschke , Robert Brunngräber

We report Herschel and AKARI photometric observations at far-infrared (FIR) wavelengths of the debris disk around the F3V star HD 15407A, in which the presence of an extremely large amount of warm dust (~500-600 K) has been suggested by…

Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system's counterparts are the asteroid and Edgeworth-Kuiper belts. The aim of this paper is to provide…

We report basic far-infrared (FIR) properties of eight blue compact dwarf galaxies (BCDs) observed by AKARI. We measure the fluxes at the four FIS bands (wavelengths of 65 um, 90 um, 140 um, and 160 um). Based on these fluxes, we estimate…

天体物理学 · 物理学 2017-01-18 Hiroyuki Hirashita , Hidehiro Kaneda , Takashi Onaka , Toyoaki Suzuki

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 present results from the earliest observations of DEBRIS, a Herschel Key Programme to conduct a volume- and flux-limited survey for debris discs in A-type through M-type stars. PACS images (from chop/nod or scan-mode observations) at 100…

We report the observations of 12 globular clusters with the AKARI/FIS. Our goal is to search for emission from the cold dust within clusters. We detect diffuse emissions toward NGC 6402 and 2808, but the IRAS 100-micron maps show the…

天体物理学 · 物理学 2017-01-18 N. Matsunaga , H. Mito , Y. Nakada , H. Fukushi , T. Tanabé , Y. Ita , H. Izumiura , M. Matsuura , T. Ueta , I. Yamamura

We compile a sample of 341 binary and multiple star systems with the aim of searching for and characterising Kuiper belt-like debris discs. The sample is assembled by combining several smaller samples studied in previously published work…

地球与行星天体物理 · 物理学 2019-07-17 Ben Yelverton , Grant M. Kennedy , Kate Y. L. Su , Mark C. Wyatt

We report the detection of a ring of warm dust in the edge-on disk surrounding HD 32297 with the Gemini-N/MICHELLE mid-infrared imager. Our N'-band image shows elongated structure consistent with the orientation of the scattered-light disk.…

天体物理学 · 物理学 2009-11-13 Michael P. Fitzgerald , Paul G. Kalas , James R. Graham