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8-13 μm dust emission features in Galactic bulge planetary nebulae

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 327:3 (2001) 744-750

Authors:

S Casassus, PF Roche, DK Aitken, CH Smith
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Deep Optical and Near-IR Observations of the XMM/Chandra Regions in ELAIS

Chapter in Deep Fields, Springer Nature (2001) 298-298

Authors:

Eduardo A González-Solares, I Pérez-Fournon, R McMahon, C Sabbey, O Almaini, C Willott, F Cabrera-Guerra, P Ciliegi, A Lawrence, B Mann, S Oliver, M Rowan-Robinson, S Serjeant, A Verma
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Design and construction of a fiber bundle connector using microlenses

OPTICAL ENGINEERING 40:12 (2001) 2709-2717

Authors:

DQ Ren, R Sharples, JR Allington-Smith, GN Dodsworth, DJ Robertson, G Dalton
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Do luminous elliptical galaxies have young disks?

ASTROPHYSICS AND SPACE SCIENCE 277 (2001) 341-341

Authors:

RM McDermid, H Kuntschner, RL Davies
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Effects of anisotropy on the central dark mass in NGC 3115. New results from integral field spectroscopy

ESO ASTROPHY SYMP (2001) 88-90

Authors:

SW Anders, N Thatte, R Genzel

Abstract:

We report new results on the stellar kinematics and the mass distribution of the galaxy NGC 3115 based on NIR integral field spectroscopic data. Investigations using long slit spectroscopic data have yielded strong evidence for the presence of a massive dark object of ca. 10(9) solar masses. NGC 3115 therefore appears to be a prominent candidate for hosting a black hole in its center. We demonstrate that with integral field spectroscopy the rotation and velocity dispersion can be much better constrained by sampling in both spatial dimensions. This yields revised and more secure results.
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