Dusty Circumstellar Disks

By B. Zuckerman. 2001

161 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/4f48509a99569899c1239b8334b412da135b2d31

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In Astronomy and Astrophysics

1. J. Farihi
2. B. Bowler
3. B. Zuckerman
4. M. C. Wyatt
5. G. Herczeg
6. Eric Mamajek
7. D. Wilner
8. Inseok Song

Citations in the corpus

• Toward Planetesimals in the Disk around TW Hydrae: 3.5 Centimeter Dust Emission (2005, background): “Recently recognized nearby stellar associations offer prime targets for observations to address the evolution of dust toward planets (Zuckerman 2001).”
• Collisional Cascades in Planetesimal Disks. II. Embedded Planets (2003, unknown): “This range is comparable to dust masses derived from observations of debris disks (Backman & Paresce 1993; Lagrange et al. 2000; Zuckerman 2001; Wyatt, Dent, & Greaves 2003).”
• INFRARED SIGNATURES OF DISRUPTED MINOR PLANETS AT WHITE DWARFS (2009, unknown): “…Leicester, University Road, Leicester LE1 7RH, UK; jf123@star.le.ac.uk 2Department of Physics & Astronomy, University of California, 430 Portola Plaza, Los Angeles, CA 90095; jura,ben@astro.ucla.edu 3Gemini Observatory, Northern Operations, 670 North A’ohoku Place, Hilo, HI 96720 (Zuckerman 2001).”
• A Tidally Disrupted Asteroid around the White Dwarf G29-38 (2003, background): “The origin of these warm grains which must be close to the white dwarf is an unsolved mystery (Zuckerman 2001).”
• Nearby Debris Disk Systems with High Fractional Luminosity Reconsidered (2006, background): “Since the infrared excess from early B-type stars might be due to free-free emission (Zuckerman 2001), the sample was limited to spectral types later than B9 in both catalogs.”
• Imaging Extrasolar Giant Planets (2016, background): “Topical reviews by Zuckerman (2001), Moro-Martin et al. (2008), Wyatt (2008), Krivov (2010), and Matthews et al. (2014a) high- 7 light recent theoretical and observational progress on the formation, modeling, and evolution of debris disks.”
• Circumstellar Debris and Pollution at White Dwarf Stars (2016, background): “It can be useful to consider debris disks as the entire planetary system, minus the planets; for detailed observational and theoretical reviews of debris disk phenomena, see Zuckerman (2001) and Wyatt (2008).”
• THE TUCANA/HOROLOGIUM, COLUMBA, AB DORADUS, AND ARGUS ASSOCIATIONS: NEW MEMBERS AND DUSTY DEBRIS DISKS (2011, methodology): “On an Astar color-magnitude diagram (Figure 5 in Zuckerman 2001), the F0-type primary lies low thus suggesting a young age.”
• Dust Dynamics, Surface Brightness Profiles, and Thermal Spectra of Debris Disks: The Case of AU Microscopii (2005, background): ““Debris disks” surrounding young stars are composed of optically thin dust (see the reviews by Artymowicz 2000; Lagrange, Backman, & Artymowicz 2000; Zuckerman 2001).”
• The Far-Ultraviolet Spectrum of TW Hydrae. I. Observations of H2 Fluorescence (2002, methodology): “Millimeter wave measurements of the dust continuum from the outer disk can be used to estimate the disk mass, assuming a dust-to-gas ratio (see review by Zuckerman 2001).”
• Spitzer IRS Spectroscopy of IRAS-discovered Debris Disks (2006, background): “Debris disks are dusty, gas-poor disks around main sequence stars (Backman & Paresce 1993; Lagrange et al. 2000; Zuckerman 2001).”
• NEW DEBRIS DISKS AROUND YOUNG, LOW-MASS STARS DISCOVERED WITH THE SPITZER SPACE TELESCOPE (2009, unknown): “…a flux-limited survey could partially account for this apparent difference in disk frequency and disk lifetime; debris disks around K and M dwarfs are thought to be relatively colder and fainter than around solartype stars, due to the lower stellar luminosities (Rhee et al. 2007; Zuckerman 2001).”
• Variations on Debris Disks: Icy Planet Formation at 30-150 AU for 1-3 M☉ Main-Sequence Stars (2008, background): “…(ISO), and Spitzer Space Telescope have revealed substantial mid-infrared (mid-IR) excesses associated with hundreds of normal mainsequence stars (e.g., Backman & Paresce1993; Habing et al. 2001; Zuckerman 2001; Rieke et al. 2005; Bryden et al. 2006;Moór et al. 2006; Rhee et al. 2007a).”
• Young Stars Near the Sun (2004, methodology): “Whether this source is physically related to β Pic has been unclear (Zuckerman 2001).”
• The Far-Ultraviolet Spectra of TW Hydrae. II. Models of H2 Fluorescence in a Disk (2004, methodology): “The extent and mass of dust in disks have been determined from IR spectral energy distributions (SEDs) and imaging (see review by Zuckerman 2001).”