Transitional Disk

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Left picture: Transitional disk around the star LkCa15, right part of the picture of the dust-free inner hole with the marked location of the star

A Transitional Disk ( German translation: interface washer ) is a protoplanetary disk to a young stellar object with a dust-free inner hole or gap in the spacing of a few astronomical units ; in its outer area, corresponding to a radius of more than 10 AU, the pane is still rich in gas and dust. Transitional disks are also referred to by some authors as transition disks , weak disks , anemic disks (pale disks) or weak excess disks . They make up about 15 percent of the population of the protoplanetary disks.

One or more gaps in protoplanetary disks as well as transition disks, the inner area of ​​which is almost completely free of dust, could be observed with the help of interferometric observations in nearby star formation regions such as the Taurus - Auriga complex. An accretion of gas onto the young star can still be detected in many cases.

At T-Tauri stars

Among the T-Tauri stars there is a group with a different spectral energy distribution : while the majority show a pronounced infrared excess in the entire range of infrared radiation , no excess can be detected in the near infrared in the range of 5 to 50 micrometers for some ; instead, an energy distribution like that of the photosphere of older stars is observed here. At longer wavelengths there is again a clear excess of infrared radiation. T-Tauri stars with transitional disks have a characteristic age of less than 10 million years.

Educational mechanisms

The following mechanisms are discussed for the dissolution of the inner parts of a protoplanetary disk:

Examples

Transitional disks have been proven to be

  • LkCa 15 with the planet LkCa 15b
  • DM dew
  • GM Aur
  • UX Tau A.

Individual evidence

  1. ^ S. Bruderer: Survival of molecular gas in cavities of transition disks (I. CO) . In: Astrophysics. Solar and Stellar Astrophysics . 2013, arxiv : 1308.2966v1 .
  2. Andrea Isella, Laura M. Pe'rez, John M. Carpenter, Luca Ricci, Sean Andrews, Katherine Rosenfeld: An azimuthal asymmetry in the LkHa 330 disk . In: Astrophysics. Solar and Stellar Astrophysics . 2013, arxiv : 1307.5848v1 .
  3. ^ Tobias WA Müller, Wilhelm Kley: Modeling Accretion in Transitional Disks . In: Astrophysics. Solar and Stellar Astrophysics . 2013, arxiv : 1310.4398v1 .
  4. Aurora Sicilia-Aguilar, Jinyoung Serena Kim, Andrej Sobolev, Konstantin Getman, Thomas Henning, Min Fang: The low-mass stellar population in the young cluster Tr37: Disk evolution, accretion, and environment . In: Astrophysics. Solar and Stellar Astrophysics . 2013, arxiv : 1308.0114v1 .
  5. ^ Jack Dobinson, Zoë M. Leinhardt, Sarah E. Dodson-Robinson, Nick A. Teanby: Hiding in the Shadows: Searching for Planets in Pre-transitional and Transitional Disks . In: Astrophysics. Solar and Stellar Astrophysics . 2013, arxiv : 1309.6480v2 .