Generation of radiative knots in a randomly pulsed protostellar jet: I. Dynamics and energetics

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Bonito, R ^a,b   Orlando, S ^b   Peres, G ^a,b   Eisloffel J ^c   Miceli, M ^a,b   Favata, F ^d  

^a UNIVERSITY OF PALERMO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c Thüringer Landessternwarte ^*  (Germany)

^d EUROPEAN SPACE AGENCY   (France)

Author keywords

Herbig Haro objects; Hydrodynamics; ISM: jets and outflows; X rays: ISM

Indexed keywords

A-TRAIN; AMBIENT MEDIUM; AXISYMMETRIC; COMPLEX INTERACTION; CURRENT MODELS; DIFFERENT SPEED; EXPONENTIAL DISTRIBUTIONS; HERBIG-HARO OBJECTS; HIGH-SPEED; HYDRODYNAMIC INSTABILITIES; ISM: JETS AND OUT FLOW; JET AXIS; MODEL RESULTS; MUTUAL INTERACTION; NUMERICAL SIMULATION; OPTICAL BANDS; PHYSICAL MECHANISM; PROPER MOTION; RADIATIVE LOSS; RANDOM VELOCITY; RATE PARAMETERS; STELLAR SOURCES; SUPERSONIC SPEED; THERMAL CONDUCTION; WAVELENGTH BAND; X-RAYS: ISM;

FLUID DYNAMICS; HYDRODYNAMICS; MORPHOLOGY; NUMERICAL METHODS; STARS; X RAYS;

SUPERSONIC AERODYNAMICS;

EID: 79952850921     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913595     Document Type: Article

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