Hubble Space Telescope Observations of the Disk and Jet of HH 30

@article{Burrows1996HubbleST,
  title={Hubble Space Telescope Observations of the Disk and Jet of HH 30},
  author={Christopher J. Burrows and Karl R. Stapelfeldt and A. M. Watson and John E. Krist and Gilda E Ballester and John T. Clarke and David Crisp and John S. Gallagher and Richard E. Griffiths and J. Jeff Hester and John G. Hoessel and Jon A. Holtzman and Jeremy Mould and Paul A. Scowen and John Terry Trauger and James A. Westphal},
  journal={The Astrophysical Journal},
  year={1996},
  volume={473},
  pages={437-451}
}
HH 30 in Taurus has been imaged with the Hubble Space Telescope WFPC2. The images show in reflected light a flared disk with a radius of about 250 AU that obscures the protostar. The disk resembles detailed accretion disk models that constrain its density distribution and show that its inclination is less than 10 degrees. There are bipolar emission-line jets perpendicular to the disk, a very clear demonstration of the standard paradigm for accretion disk and jet systems. However, asymmetries in… 
A variable asymmetry in the circumstellar disk of HH 30
We report Hubble Space Telescope observations of variability within the reflection nebulosity of HH 30, a compact bipolar nebula that is a nearly edge-on accretion disk system. A dramatic lateral
Hubble Space Telescope WFPC2 Imaging of the Disk and Jet of HV Tauri C
We have obtained Hubble Space Telescope (HST) WFPC2 images of the HV Tauri young triple system. The tertiary star appears as a compact bipolar nebula at visual wavelengths as already known in the
Resolving the circumbinary dust disk surrounding HH 30
Context. The jet-disk connection is an important part of the star formation process. HH 30 is a rare and beautiful example of a system exhibiting a flared edge-on disk, an optical jet and a CO
Proper Motions in the Knotty, Bipolar Jet in Henize 2-90
Using second-epoch Hubble Space Telescope imaging of the unusual, bipolar jet source He 2-90, we have discovered proper motions of 003 yr-1 in the jet knots. Combining the proper motion with the
Collimation, Proper Motions, and Physical Conditions in the HH 30 Jet from Hubble Space Telescope Slitless Spectroscopy*
We present STIS spectral images of the HH 30 stellar jet taken through a wide slit over two epochs. The jet is unresolved spectrally, so the observations produce emission-line images for each line in
Hubble Space Telescope Imaging of the Disks and Jets of Taurus Young Stellar Objects
We report on Hubble Space Telescope imaging of eleven young stellar objects in the nearby Taurus molecular clouds. The high spatial resolution and stable point spread function of HST reveal important
Millimeter Properties of the Protoplanetary Disk Surrounding HH 30
HH30 is a well-known PMS star located in the Taurus molecular cloud, at a distance of ~140 pc. Burrows et al. (1996) [1] obtained spectacular images with the Hubble Space Telescope, revealing i) a
Probing the inner part of protoplanetary disks with the VLTI
Young stellar objects offer a rich circumstellar environment, indirectly revealed by photometry, spectroscopy and imaging, such as accretion disks, stellar companions, optical jets, stellar winds,
High-Resolution Near-Infrared Images and Models of the Circumstellar Disk in HH 30
We present Hubble Space Telescope near-infrared camera and multiobject spectrometer observations of the reflection nebulosity associated with the T Tauri star HH 30. The images show the
Plateau de Bure interferometer observations of the disk and outflow of HH 30
HH30 is a well-known Pre-Main-Sequence star in Taurus. HST observations have revealed a flared, edge-on disk driving a highly-collimated optical jet, making this object a case study for the
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