Towards the Rosetta Stone of planet formation

G. Maciejewski; R. Neuhäuser; R. Errmann; M. Mugrauer; Ch Adam; A. Berndt; T. Eisenbeiss; S. Fiedler; Ch Ginski; M. Hohle; U. Kramm; C. Marka; M. Moualla; T. Pribulla; St Raetz; T. Roell; T. O. B. Schmidt; M. Seeliger; I. Spaleniak; N. Tetzlaff; L. Trepl

doi:10.1051/epjconf/20101104006

Towards the Rosetta Stone of planet formation

G. Maciejewski, R. Neuhäuser, R. Errmann, M. Mugrauer, Ch Adam, A. Berndt, T. Eisenbeiss, S. Fiedler, Ch Ginski, M. Hohle, U. Kramm, C. Marka, M. Moualla, T. Pribulla, St Raetz, T. Roell, T. O. B. Schmidt, M. Seeliger, I. Spaleniak, N. TetzlaffL. Trepl

Physics

Research output: Chapter in Book or Conference Publication/Proceeding › Conference Publication

1 Citation (Scopus)

Abstract

Transiting exoplanets (TEPs) observed just ~10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g. time-scales (planet formation would then be possible within 10 Myrs), the radius of the planet could indicate whether planets form by gravitational collapse (being larger when young) or accretion growth (being smaller when young). We present a survey, the main goal of which is to find and then characterise TEPs in very young open clusters.

...

Original language	English
Title of host publication	European Physical Journal Web of Conferences
DOIs	https://doi.org/10.1051/epjconf/20101104006
Publication status	Published - Feb 2011

Access to Document

10.1051/epjconf/20101104006

Cite this

Maciejewski, G., Neuhäuser, R., Errmann, R., Mugrauer, M., Adam, C., Berndt, A., Eisenbeiss, T., Fiedler, S., Ginski, C., Hohle, M., Kramm, U., Marka, C., Moualla, M., Pribulla, T., Raetz, S., Roell, T., Schmidt, T. O. B., Seeliger, M., Spaleniak, I., ... Trepl, L. (2011). Towards the Rosetta Stone of planet formation. In European Physical Journal Web of Conferences https://doi.org/10.1051/epjconf/20101104006

@inproceedings{2ccdf52368aa42afb6f35ff3454b7907,

title = "Towards the Rosetta Stone of planet formation",

abstract = "Transiting exoplanets (TEPs) observed just \textasciitilde{}10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g. time-scales (planet formation would then be possible within 10 Myrs), the radius of the planet could indicate whether planets form by gravitational collapse (being larger when young) or accretion growth (being smaller when young). We present a survey, the main goal of which is to find and then characterise TEPs in very young open clusters. ...",

author = "G. Maciejewski and R. Neuh{\"a}user and R. Errmann and M. Mugrauer and Ch Adam and A. Berndt and T. Eisenbeiss and S. Fiedler and Ch Ginski and M. Hohle and U. Kramm and C. Marka and M. Moualla and T. Pribulla and St Raetz and T. Roell and Schmidt, \{T. O. B.\} and M. Seeliger and I. Spaleniak and N. Tetzlaff and L. Trepl",

year = "2011",

month = feb,

doi = "10.1051/epjconf/20101104006",

language = "English",

booktitle = "European Physical Journal Web of Conferences",

}

Maciejewski, G, Neuhäuser, R, Errmann, R, Mugrauer, M, Adam, C, Berndt, A, Eisenbeiss, T, Fiedler, S, Ginski, C, Hohle, M, Kramm, U, Marka, C, Moualla, M, Pribulla, T, Raetz, S, Roell, T, Schmidt, TOB, Seeliger, M, Spaleniak, I, Tetzlaff, N & Trepl, L 2011, Towards the Rosetta Stone of planet formation. in European Physical Journal Web of Conferences. https://doi.org/10.1051/epjconf/20101104006

TY - GEN

T1 - Towards the Rosetta Stone of planet formation

AU - Maciejewski, G.

AU - Neuhäuser, R.

AU - Errmann, R.

AU - Mugrauer, M.

AU - Adam, Ch

AU - Berndt, A.

AU - Eisenbeiss, T.

AU - Fiedler, S.

AU - Ginski, Ch

AU - Hohle, M.

AU - Kramm, U.

AU - Marka, C.

AU - Moualla, M.

AU - Pribulla, T.

AU - Raetz, St

AU - Roell, T.

AU - Schmidt, T. O. B.

AU - Seeliger, M.

AU - Spaleniak, I.

AU - Tetzlaff, N.

AU - Trepl, L.

PY - 2011/2

Y1 - 2011/2

N2 - Transiting exoplanets (TEPs) observed just ~10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g. time-scales (planet formation would then be possible within 10 Myrs), the radius of the planet could indicate whether planets form by gravitational collapse (being larger when young) or accretion growth (being smaller when young). We present a survey, the main goal of which is to find and then characterise TEPs in very young open clusters. ...

AB - Transiting exoplanets (TEPs) observed just ~10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g. time-scales (planet formation would then be possible within 10 Myrs), the radius of the planet could indicate whether planets form by gravitational collapse (being larger when young) or accretion growth (being smaller when young). We present a survey, the main goal of which is to find and then characterise TEPs in very young open clusters. ...

U2 - 10.1051/epjconf/20101104006

DO - 10.1051/epjconf/20101104006

M3 - Conference Publication

BT - European Physical Journal Web of Conferences

ER -

Towards the Rosetta Stone of planet formation

Abstract

Access to Document

Fingerprint

Cite this