Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265l..71m&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 265, Feb. 15, 1983, p. L71-L75. Deutsche Forschungsgemeinschaft
Astronomy and Astrophysics
Astrophysics
82
Herbig-Haro Objects, Main Sequence Stars, Stellar Mass Ejection, T Tauri Stars, High Resolution, Line Spectra, Red Shift, Stellar Spectra, Stellar Winds
Scientific paper
A new Herbig-Haro object, designated HH 32C, has been discovered near the T Tauri star AS 353A. HH 32C is aligned on the opposite side of AS 353A from two previously known HH objects 32A and B. The emission-line spectrum of HH 32C shows high-velocity blueshifted material moving at speeds (350-400 km s-1) comparable to the high-velocity redshifted material in HH 32A and B. Thus, this represents the second case (after HH 1 and 2 emanating from the Cohen-Schwartz star) in which HH objects clearly trace a high-velocity, well-collimated bipolar outflow from the immediate vicinity of a visible pre-main-sequence object.
Mundt Reinhard
Stocke John
Stockman Hervey S.
No associations
LandOfFree
Jets from pre-main-sequence stars - As 353A and its associated Herbig-Haro objects 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 Jets from pre-main-sequence stars - As 353A and its associated Herbig-Haro objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Jets from pre-main-sequence stars - As 353A and its associated Herbig-Haro objects will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1305899