Structure and evolution of extra-galactic sources and their relationship to the background radiations

Projektinformationen

ID Finanzhilfevereinbarung: CIPD940028

Startdatum 1 Dezember 1994

Enddatum 31 August 1996

Finanziert unter

• Scientific and technological cooperation between the European Community and European non-member countries, 1992-

Gesamtkosten € 0,00

EU-Beitrag Keine Daten

Koordiniert durch

Osservatorio Astronomico di Padova
Italy

Ziel

WE PROPOSE A SYSTEMATIC STUDY OF THE BROAD LINE PROFILES IN AGN. STUDIES OF THE EMISSION LINE PROFILES PROVIDE INFORMATION ON THE SPATIAL AND KINEMATIC PROPERTIES OF THE EMITTING GAS. MOREOVER STATISTICAL DATA ON PROFILE PROPERTIES CAN PROVIDE DIRECT CONSTRAINTS ON MODELS OF THE EMITTING REGION.
WE SHALL PUT SPECIAL EMPHASIS ON LINE ASYMMETRIES, THAT CAN SHED LIGHT ON THE ACCRETION DISK MODEL FOR THE CENTRAL ENGINE OF AGN, AND ON VELOCITY DIFFERENCES THAT HAVE BEEN OBSERVED AMONG THE BROAD LINE REGION LINES AND BETWEEN THE BRL LINES AND THE NARROW LINE REGION LINES.
OUR GOALS ARE THREEFOLD: 1) TO EFFECTIVELY PARAMETRIZE THE LINE PROFILES; 2) TO USE THE DERIVED PARAMETERS TO CONSTRAIN CURRENT AGN MODELS; 3) To SEARCH FOR CORRELATIONS AMONG THE DERIVED PARAMETERS, OR WITH OTHER OBSERVABLES, THAT MIGHT PROVIDE FURTHER CLUES TO THE AGN PROCESS.

Programm/Programme

• IC-PECO/COPERNICUS - Scientific and technological cooperation between the European Community and European non-member countries, 1992-

Thema/Themen

• 0401 - CEEC participation in HUMAN CAPITAL & MOBILITY programme (NETWORKS)

Aufforderung zur Vorschlagseinreichung

Data not available

Finanzierungsplan

CSC - Cost-sharing contracts

Koordinator

Osservatorio Astronomico di Padova

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• Adresse: Vicolo dell'Osservatorio 5 ; 35122 Padova ; Italien
• Gesamtkosten: Keine Daten

Beteiligte (1)

University of Ljubljana

Slowenien

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• Adresse: 19,Jadranska ; 1000 Ljubljana
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