Physical structure and dust reprocessing in a sample of HH jets

Astronomy and Astrophysics

Volumn 506, Issue 2, 2009, Pages 779-788

  Podio, L ^a   Medves, S ^b   Bacciotti, F ^c   Eisloffel J ^d   Ray, T ^a  

^a DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^b UNIVERSITY OF PISA   (Italy)

^c INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^d THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

Author keywords

ISM: dust, extinction; ISM: Herbig Haro objects; ISM: jets and outflows; Stars: formation

Indexed keywords

CHARACTERISTIC EMISSION; DIAGNOSTIC TECHNIQUES; DUST CONTENT; DUST GRAINS; ELECTRON DENSITIES; EXCITATION CONDITIONS; FORBIDDEN LINES; GAS VELOCITY; GAS-PHASE ABUNDANCE; HIGH VELOCITY; HYDROGEN DENSITIES; INTERSTELLAR MEDIUMS; IONISATION; ISM: DUST, EXTINCTION; ISM: HERBIG-HARO OBJECTS; ISM: JETS AND OUTFLOWS; MOLECULAR CLOUDS; PHYSICAL CONDITIONS; PHYSICAL STRUCTURES; PLASMA CONDITIONS; SHOCK STRUCTURE; SHOCK VELOCITIES; STAR-FORMATION PROCESS; STARS: FORMATION; TEMPERATURE RANGE; TOTAL DENSITY; WEALTH OF INFORMATION;

CALCIUM; CALCIUM ALLOYS; CLOUDS; DUST; EMISSION SPECTROSCOPY; HYDROGEN; IONIZATION; STARS; TELLURIUM COMPOUNDS;

JETS;

EID: 70350439561     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912408     Document Type: Article

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