Protoplanetary Worlds at the Astronomical Unit Scale. First Step towards Aperture Synthesis Images

J. Berger; J. Monnier; R. Millan-Gabet; F. Malbet; M. Benisty; E. Pedretti; W. Traub

Protoplanetary Worlds at the Astronomical Unit Scale. First Step towards Aperture Synthesis Images

J. Berger, J. Monnier, R. Millan-Gabet, F. Malbet, M. Benisty, E. Pedretti, W. Traub

School of Engineering & Physical Sciences

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Optical interferometry has started to play a crucial role in the field of star formation. In particular, it offers a unique opportunity to observe protoplanetary disks at a spatial scale where planets may be forming. We present here some of the most recent discoveries in this field putting the emphasis on the progress towards direct imaging of proto-planetary worlds at the astronomical unit scale. In particular we develop our use of the IOTA/IONIC3 interferometer to measure closure phase quantities, a powerful observable to quantify the degree of skewness of the infrared emission at spatial scales corresponding to the internal part of the disk.

Original language	English
Title of host publication	Visions for Infrared Astronomy, Instrumentation, Mesure, Métrologie
Editors	V. Coudé du Foresto, D. Rouan, G. Rousset
Pages	245-250
Number of pages	6
Volume	6
Edition	1-4
Publication status	Published - 2006

Keywords

pre-main sequence stars, protoplanetary disks, long baseline infrared interferome- try, closure phases, T Tauri, Herbig AeBe, Fu Orionis.

Cite this

@inproceedings{c4418cfa8f304599bd1c8fd87e954897,

title = "Protoplanetary Worlds at the Astronomical Unit Scale. First Step towards Aperture Synthesis Images",

abstract = "Optical interferometry has started to play a crucial role in the field of star formation. In particular, it offers a unique opportunity to observe protoplanetary disks at a spatial scale where planets may be forming. We present here some of the most recent discoveries in this field putting the emphasis on the progress towards direct imaging of proto-planetary worlds at the astronomical unit scale. In particular we develop our use of the IOTA/IONIC3 interferometer to measure closure phase quantities, a powerful observable to quantify the degree of skewness of the infrared emission at spatial scales corresponding to the internal part of the disk.",

keywords = "pre-main sequence stars, protoplanetary disks, long baseline infrared interferome- try, closure phases, T Tauri, Herbig AeBe, Fu Orionis.",

author = "J. Berger and J. Monnier and R. Millan-Gabet and F. Malbet and M. Benisty and E. Pedretti and W. Traub",

year = "2006",

language = "English",

volume = "6",

pages = "245--250",

editor = "\{Coud{\'e} du Foresto\}, V. and D. Rouan and G. Rousset",

booktitle = "Visions for Infrared Astronomy, Instrumentation, Mesure, M{\'e}trologie",

edition = "1-4",

}

Protoplanetary Worlds at the Astronomical Unit Scale. First Step towards Aperture Synthesis Images. / Berger, J.; Monnier, J.; Millan-Gabet, R. et al.
Visions for Infrared Astronomy, Instrumentation, Mesure, Métrologie. ed. / V. Coudé du Foresto; D. Rouan; G. Rousset. Vol. 6 1-4. ed. 2006. p. 245-250.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Protoplanetary Worlds at the Astronomical Unit Scale. First Step towards Aperture Synthesis Images

AU - Berger, J.

AU - Monnier, J.

AU - Millan-Gabet, R.

AU - Malbet, F.

AU - Benisty, M.

AU - Pedretti, E.

AU - Traub, W.

PY - 2006

Y1 - 2006

N2 - Optical interferometry has started to play a crucial role in the field of star formation. In particular, it offers a unique opportunity to observe protoplanetary disks at a spatial scale where planets may be forming. We present here some of the most recent discoveries in this field putting the emphasis on the progress towards direct imaging of proto-planetary worlds at the astronomical unit scale. In particular we develop our use of the IOTA/IONIC3 interferometer to measure closure phase quantities, a powerful observable to quantify the degree of skewness of the infrared emission at spatial scales corresponding to the internal part of the disk.

AB - Optical interferometry has started to play a crucial role in the field of star formation. In particular, it offers a unique opportunity to observe protoplanetary disks at a spatial scale where planets may be forming. We present here some of the most recent discoveries in this field putting the emphasis on the progress towards direct imaging of proto-planetary worlds at the astronomical unit scale. In particular we develop our use of the IOTA/IONIC3 interferometer to measure closure phase quantities, a powerful observable to quantify the degree of skewness of the infrared emission at spatial scales corresponding to the internal part of the disk.

KW - pre-main sequence stars, protoplanetary disks, long baseline infrared interferome- try, closure phases, T Tauri, Herbig AeBe, Fu Orionis.

M3 - Conference contribution

VL - 6

SP - 245

EP - 250

BT - Visions for Infrared Astronomy, Instrumentation, Mesure, Métrologie

A2 - Coudé du Foresto, V.

A2 - Rouan, D.

A2 - Rousset, G.

ER -

Protoplanetary Worlds at the Astronomical Unit Scale. First Step towards Aperture Synthesis Images

Abstract

Keywords

Fingerprint

Cite this