SIMBAD references

2004ApJ...601L..91T - Astrophys. J., 601, L91-L94 (2004/January-3)

H2Emission nebulosity associated with KH 15D.

TOKUNAGA A.T., DAHM S., GASSLER W., HAYANO Y., HAYASHI M., IYE M., KANZAWA T., KOBAYASHI N., KAMATA Y., MINOWA Y., NEDACHI K., OYA S., PYO T.-S., SAINT-JACQUES D., TERADA H., TAKAMI H. and TAKATO N.

Abstract (from CDS):

An H2emission filament is found in close proximity to the unique object KH 15D using the adaptive optics system of the Subaru Telescope. The morphology of the filament, the presence of spectroscopic outflow signatures observed by Hamilton et al., and the detection of extended H2emission from KH 15D by Deming, Charbonneau, & Harrington suggest that this filament arises from shocked H2in an outflow. The filament extends about 15" to the north of KH 15D.

Abstract Copyright: ∼

Journal keyword(s): ISM: Jets and Outflows - Stars: Planetary Systems - Stars: Individual: Alphanumeric: KH 15D - Stars: Pre-Main-Sequence

Nomenclature: Fig.1, Table 1: [TDG2004] Filament N=1, [TDG2004] Knot A (Nos A-B).

CDS comments: KH 15D = Cl* NGC 2264 VVO 15D

Simbad objects: 8

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