Observations of outflows and disks in pre-main sequence systems

Details Observations of outflows and disks in pre-main sequence systems Observations of outflows and disks in pre-main sequence systems

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..523b&link_type=abstract

Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astrophysics

Pre-Main Sequence Objects, Young Stellar Objects And Protostars, Accretion And Accretion Disks, Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds

Scientific paper

The high angular resolution of Hubble Space Telescope has provided
stunning evidence for accretion disks around low mass stars and revealed
the detailed structure of stellar jets. Large format CCD detectors have
been used to show that outflows from young stars can extend parsecs from
their sources.

Affiliated with

Also associated with

No associations

Rating

Observations of outflows and disks in pre-main sequence systems does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Observations of outflows and disks in pre-main sequence systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of outflows and disks in pre-main sequence systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1602328