Spectral energy distributions of accreting protoplanets

Research output: Contribution to journalArticle

19 Citations (Scopus)

Abstract

Planets are often invoked as the cause of inferred gaps or inner clearings in transition disks. These putative planets would interact with the remnant circumstellar disk, accreting gas and generating substantial luminosity. Here I explore the expected appearance of accreting protoplanets at a range of evolutionary states. I compare synthetic spectral energy distributions with the handful of claimed detections of substellar-mass companions in transition disks. While observed fluxes of candidate companions are generally compatible with accreting protoplanets, challenges remain in reconciling the extended structure inferred in observed objects with the compact emission expected from protoplanets or circumplanetary disks. I argue that a large fraction of transition disks should harbor bright protoplanets, and that more may be detected as larger telescopes open up additional parameter space.

Original languageEnglish (US)
Article numberL4
JournalAstrophysical Journal Letters
Volume803
Issue number1
DOIs
StatePublished - Apr 10 2015

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protoplanets
spectral energy distribution
planet
energy
harbor
planets
gas
clearing
harbors
luminosity
distribution
telescopes
causes
gases
detection
parameter

Keywords

  • accretion, accretion disks
  • disk interactions
  • planet
  • planets and satellites: formation
  • protoplanetary disks

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Spectral energy distributions of accreting protoplanets. / Eisner, Joshua A.

In: Astrophysical Journal Letters, Vol. 803, No. 1, L4, 10.04.2015.

Research output: Contribution to journalArticle

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