A Symmetric Inner Cavity in the HD 141569A Circumstellar Disk
Ground-based Near-Infrared Imaging of the HD 141569 Circumstellar Disk
High-contrast Near-infrared Polarization Imaging of MWC480
HST/NICMOS2 coronagraphic observations of the circumstellar environment of three old PMS stars: HD 100546, SAO 206462 and MWC 480
HST/NICMOS2 observations of the HD 141569 A circumstellar disk
Locating the Accretion Footprint on a Herbig Ae Star: MWC 480
Multiple spiral patterns in the transitional disk of HD 100546
Near-infrared imaging polarimetry of dusty young stars
Revealing the Structure of a Pre-Transitional Disk: The Case of the Herbig F Star SAO 206462 (HD 135344B)
Spiral Arms in Disks: Planets or Gravitational Instability?
Very Large Telescope/NACO Polarimetric Differential Imaging of HD100546--Disk Structure and Dust Grain Properties between 10 and 140 AU
Why circumstellar disks are so faint in scattered light: the case of HD 100546
Instrument
NICMOS/NIC1, NICMOS/NIC2, NICMOS/NIC3
Temporal Coverage
1998-02-24T16:31:15Z/1998-11-09T21:02:15Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Lagrange comma Anne-Marie, 1999, 'Investigating the missing link between disks around Pre Main Sequence and Main Sequence stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-wyp1w16
