869 research outputs found

    Infrared observations of OB star formation in NGC 6334

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    Infrared photometry and maps from 2 to 100 microns are presented for three of the principal far infrared sources in NGC 6334. Each region is powered by two or more very young stars. The distribution of dust and ionized gas is probably strongly affected by the presence of the embedded stars; one of the sources is a blister H II region, another has a bipolar structure, and the third exhibits asymmetric temperature structure. The presence of protostellar objects throughout the region suggests that star formation has occurred nearly simultaneously in the whole molecular cloud rather than having been triggered sequentially from within

    Nuclear bars and blue nuclei within barred spiral galaxies

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    Multicolour near IR photometry for a sample of 32 large barred spiral galaxies is presented. By applying ellipse fitting techniques, we identify significant isophote twists with respect to the primary bar axis in the nuclear regions of ∼\sim70 \%\ of the sample. These twists are identified in galaxies as late as SBbc and are clearly distinguishable from spiral arm morphology. At most seven of the galaxies with isophote twists are inferred to possess secondary (nuclear) bars, the axis ratios of which appear to correlate with morphological type. The remainder may result from triaxial bulges, or from oblate bulges misaligned with the primary bar. The near IR colour distributions in these data show evidence for (red) circumnuclear star forming rings in 4 galaxies. The majority of the sample (19) also possess striking blue nuclear regions, bluer than typical old stellar populations by ∼\sim0.3 mag. in (J--H) and ∼\sim0.23 mag. in (H--K). Such blue colours do not appear to correlate with the presence of nuclear rings or pseudo--rings, nor with the activity of the host galaxy (as determined from emission--line spectroscopic characteristics). Several mechanisms to explain this blue colour are considered.Comment: 24 pages plain LaTex( including table captions), 5 tables and 18 figures. Accepted for publication in MNRAS. Paper and tables available via anonymous ftp://143.167.4.101/pub/papers as sqiid-paper.tex and table1,2,3.tex, table4.ps, table5.ps. Figures available as postcript upon request to first Autho

    PHYS 202-001: Introductory Astronomy and Cosmology

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    PHYS 202-001: Introductory Astronomy and Cosmology

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    The Question of Auckland’s Civic Building

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    This article examines recent and current controversy over the Civic Administration Building (1954- 1966) in Auckland, New Zealand. Unoccupied since the end of 2014, the building’s future is uncertain. Its heritage value is widely recognized by heritage professionals and commentators. Yet Auckland Council, the building’s owner and former occupier, does not recognize its significance and has not scheduled it as a heritage building on its district plan. To the contrary, it has floated the possibility of demolishing it. This article considers the building’s history, significance and possible futures

    PHYS 202-002: Introductory Astronomy and Cosmology

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    PHYS 202-001: Introductory Astronomy and Cosmology

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