Integral field optical spectroscopy using the INTEGRAL system has been used to characterize the kinematic and ionization properties of the warm gas within 2 kpc of the dust-enshrouded nucleus of Arp 220. Owing to the large internal extinction toward the nuclei, the brightest stellar and line-emitting regions observed at optical wavelengths do not
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Two-dimensional Kinematical and Ionization Structure of the Warm Gas in the Nuclear Regions of Arp 220Arribas, Santiago et al.102001
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Type Ia supernovae with and without blueshifted narrow Na I D lines - how different is their structure?
In studies on intermediate- and high-resolution spectra of Type Ia supernovae (SNe Ia), some objects exhibit narrow Na I D absorptions often blueshifted with respect to the rest wavelength within the host galaxy. The absence of these in other SNe Ia may reflect that the explosions have different progenitors: blueshifted Na I D features might be
Hachinger, S. et al.Advertised on:
102017 -
Ubiquitous seeding of supermassive black holes by direct collapse
We study for the first time the environment of massive black hole (BH) seeds (˜104-5 M⊙) formed via the direct collapse of pristine gas clouds in massive haloes (≥107 M⊙) at z > 6. Our model is based on the evolution of dark matter haloes within a cosmological N-body simulation, combined with prescriptions for the formation of BH along with both
Agarwal, Bhaskar et al.Advertised on:
102012 -
UBVRI Outburst of the Dwarf Nova AH Her
Not Available
Lazaro, C. et al.Advertised on:
101986 -
Ultracool dwarf benchmarks with Gaia primaries
We explore the potential of Gaia for the field of benchmark ultracool/brown dwarf companions, and present the results of an initial search for metal-rich/metal-poor systems. A simulated population of resolved ultracool dwarf companions to Gaia primary stars is generated and assessed. Of the order of ˜24 000 companions should be identifiable outside
Marocco, F. et al.Advertised on:
102017 -
Understanding Galactic planetary nebulae with precise/reliable nebular abundances
We compare recent precise/reliable nebular abundances - as derived from high-quality optical spectra and the most recent ICFs - in a sample of Galactic planetary nebulae (PNe) with nucleosynthesis predictions (HeCNOCl) from asymptotic giant branch (AGB) ATON models in the metallicity range Z ⊙/4 < Z < 2Z ⊙. According to the infrared dust features
García-Hernández, D. A. et al.Advertised on:
102017