ALMA REVEALS THE ANATOMY OF THE mm-SIZED DUST AND MOLECULAR GAS IN THE HD 97048 DISK

ABSTRACT Transitional disks show a lack of excess emission at infrared wavelengths due to a large dust cavity, that is often corroborated by spatially resolved observations at ∼ mm wavelengths. We present the first spatially resolved ∼ mm-wavelength images of the disk around the Herbig Ae/Be star, H...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2016-11, Vol.831 (2), p.200
Hauptverfasser:	Walsh, Catherine, Juhász, Attila, Meeus, Gwendolyn, Dent, William R. F., Maud, Luke T., Aikawa, Yuri, Millar, Tom J., Nomura, Hideko
Format:	Artikel
Sprache:	eng
Schlagworte:	ANATOMY Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY AUGER ELECTRON SPECTROSCOPY CARBON MONOXIDE CLASSIFICATION Continuum radiation COSMIC DUST Disks Dust EMISSION Emissions Image classification Infrared imaging LAYERS Molecular gases protoplanetary disks PROTOPLANETS Radial drift RESOLUTION SIMULATION STARS stars: individual (HD 97048) stars: pre-main sequence submillimeter: planetary systems SYMMETRY Visibility VISIBLE RADIATION WAVELENGTHS
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!