Evolution of the nuclear accretion disk emission in NGC 1097: Getting closer to the black hole

Astrophysical Journal

Volumn 598, Issue 2 I, 2003, Pages 956-968

  Storchi Bergmann, Thaisa ^a,b,c   Da Silva, Rodrigo Nemmen ^a   Eracleous, Michael ^b,d,e,f   Halpern, Jules P ^b,g   Wilson, Andrew S ^b,h   Filippenko, Alexei V ^i,j,k   Ruiz, Maria Teresa ^b,l   Smith, R Chris ^m   Nagar, Neil M ^b,n  

^a FEDERAL UNIVERSITY OF RIO GRANDE DO SUL   (Brazil)

^b Cerro Tololo Inter Amer Observatory   (United States)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d PENNSYLVANIA STATE UNIVERSITY   (United States)

^e KITT PEAK NATIONAL OBSERVATORY   (United States)

^f MDM Observatory   (United States)

^g Columbia University ^*  (United States)

^h UNIVERSITY OF MARYLAND   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j W M KECK OBSERVATORY   (United States)

^k University of California at Santa Cruz   (United States)

^l UNIVERSITY OF CHILE   (Chile)

^m CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

ⁿ INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

more..

Author keywords

Accretion, accretion disks; Galaxies: individual (NGC 1097); Galaxies: nuclei; Galaxies: Seyfert; Line: profiles

Indexed keywords

EID: 0345818174     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/378938     Document Type: Article

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