DQ herculis in profile: Whole earth telescope observations and smoothed particle hydrodynamics simulations of an edge-on cataclysmic variable system

Astrophysical Journal

Volumn 634, Issue 1 I, 2005, Pages 570-584

  Wood, M A ^a   Robertson, J R ^a,b,c   Simpson, J C ^d   Kawaler, S D ^e   O'Brien, M S ^e,f   Nather, R E ^g   Winget, D E ^g   Montgomery, M H ^g,h   Metcalfe, T S ^g,i   Jiang, X J ^j   Leibowitz, E M ^k   Ibbetson, P ^k   O'Donoghue, D ^l   Zola, S ^m,n   Krzesinski, J ⁿ   Pajdosz, G ⁿ   Vauclair, G ^o   Dolez, N ^o   Chevreton, M ^p   Sullivan, D J ^q   Kanaan, A ^r   Nitta, A ^s   more..

^a Florida Institute of Technology   (United States)

^b APPALACHIAN STATE UNIVERSITY   (United States)

^c Southeastern Association for Research in Astronomy   (United States)

^d KENNEDY SPACE CENTER   (United States)

^e IOWA STATE UNIVERSITY   (United States)

^f YALE UNIVERSITY   (United States)

^g UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^h UNIVERSITY OF CAMBRIDGE   (United Kingdom)

ⁱ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^j CHINESE ACADEMY OF SCIENCES   (China)

^k TEL AVIV UNIVERSITY   (Israel)

^l SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^m JAGIELLONIAN UNIVERSITY   (Poland)

ⁿ PEDAGOGICAL UNIVERSITY   (Poland)

^o OBSERVATOIRE MIDI PYRÉNÉES   (France)

^p OBSERVATOIRE DE PARIS   (France)

^q VICTORIA UNIVERSITY OF WELLINGTON   (New Zealand)

^r FEDERAL UNIVERSITY OF SANTA CATARINA   (Brazil)

^s APACHE POINT OBSERVATORY   (United States)

more..

Author keywords

Accretion, accretion disks; Binaries: close; Hydrodynamics; Novae, cataclysmic variables; Stars: individual (DQ Her)

Indexed keywords

EID: 29144464851     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/496957     Document Type: Article

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