HR Del REMNANT ANATOMY USING TWO-DIMENSIONAL SPECTRAL DATA AND THREE-DIMENSIONAL PHOTOIONIZATION SHELL MODELS
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
18/04/2012
18/04/2012
2009
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Resumo |
The HR Del nova remnant was observed with the IFU-GMOS at Gemini North. The spatially resolved spectral data cube was used in the kinematic, morphological, and abundance analysis of the ejecta. The line maps show a very clumpy shell with two main symmetric structures. The first one is the outer part of the shell seen in H alpha, which forms two rings projected in the sky plane. These ring structures correspond to a closed hourglass shape, first proposed by Harman & O'Brien. The equatorial emission enhancement is caused by the superimposed hourglass structures in the line of sight. The second structure seen only in the [O III] and [N II] maps is located along the polar directions inside the hourglass structure. Abundance gradients between the polar caps and equatorial region were not found. However, the outer part of the shell seems to be less abundant in oxygen and nitrogen than the inner regions. Detailed 2.5-dimensional photoionization modeling of the three-dimensional shell was performed using the mass distribution inferred from the observations and the presence of mass clumps. The resulting model grids are used to constrain the physical properties of the shell as well as the central ionizing source. A sequence of three-dimensional clumpy models including a disk-shaped ionization source is able to reproduce the ionization gradients between polar and equatorial regions of the shell. Differences between shell axial ratios in different lines can also be explained by aspherical illumination. A total shell mass of 9 x 10(-4) M(circle dot) is derived from these models. We estimate that 50%-70% of the shell mass is contained in neutral clumps with density contrast up to a factor of 30. CNPq[142389/2006-4] CNPq[305275] (NSF) National Science Foundation (United States) STFC Science and Technology Facilities Council (United Kingdom) National Research Council (NSERC), Canada CONICYT (Chile) Australian Research Council(Australia) Ministerio da Ciencia e Tecnologia (Brazil) MINCyT Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina) |
Identificador |
ASTRONOMICAL JOURNAL, v.138, n.6, p.1541-1556, 2009 0004-6256 http://producao.usp.br/handle/BDPI/15682 10.1088/0004-6256/138/6/1541 |
Idioma(s) |
eng |
Publicador |
IOP PUBLISHING LTD |
Relação |
Astronomical Journal |
Direitos |
closedAccess Copyright IOP PUBLISHING LTD |
Palavras-Chave | #circumstellar matter #novae, cataclysmic variables #stars: kinematics #stars: individual (HR Del) #techniques: spectroscopic #GROUND-BASED SPECTROSCOPY #NOVA RS OPHIUCHI #PLANETARY-NEBULAE #CLASSICAL NOVAE #2006 OUTBURST #X-RAY #SPACE #EVOLUTION #DELPHINI #STARS #Astronomy & Astrophysics |
Tipo |
article original article publishedVersion |