Статья

Tracing kinematical and physical asymmetries in the jet from DG Tauri B

L. PodioKapteyn Astronomical Institute, Landleven 12, 9747 AD Groningen, The NetherlandsJ. EislöffelThüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, GermanyS. MelnikovUlugh Beg Astronomical Institute, Astronomical str. 33, 700052 Tashkent, UzbekistanK. W. HodappInstitute for Astronomy, University of Hawaii, 640 N. Aohoku Place, Hilo, HI 96720, USAF. BacciottiINAF – Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy

Astronomy and Astrophysicsjournal2010en

ABI

Аннотация

Context. Jets from young stars can be highly asymmetric and have multiple velocity components.

Темы

Astrophysics and Star Formation Studies Stellar, planetary, and galactic studies Gamma-ray bursts and supernovae

Идентификаторы

DOI: 10.1051/0004-6361/201016049

Цитирования и источники

Цитирований: 2 Использованных источников: 72

Показатели — AkademScholar · Скоро