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Martins, D. H.

Publications and source records attributed to Martins, D. H..

Preliminary photometry in the nuclear region of NGC 6624

Results are presented for initial observations near the center of NGC 6624. Photoelectrically calibrated photographic photometry is used to discuss the characteristics of the nucleus and individual stars in its vicinity. The data in their present form are not conclusive, but could imply the presence of a closely bound group of stars near the cluster center. It is proposed that one or more of these stars may be binary systems similar to the model recently suggested for Cyg X-2. However, a massive object near the center cannot be ruled out.

Harvel, C. A.

Photometry of the 'Seyfert Sextet' /VV 115/ and the anonymous galaxy 1558.2 + 2100

Photometric observations of the Seyfert Sextet (VV 115) are analyzed. Apparent integrated magnitudes are derived relative to the sky brightness, and isophotal maps are given for the field. No evidence for interaction between NGC 6027 and d is found. Luminosity profiles are given for NGC 6027, a, b, and d, with the d profile having been corrected for seeing effects in one dimension. The corrected profile parameters favor the interpretation of d as a highly luminous background galaxy at its cosmological distance. The nearby anonymous galaxy 1558.2 + 2100 is similarly studied, with no clear evidence of photometric peculiarities detected. Its interaction with the Seyfert Sextet appears to be excluded.

Martins, D. H.

Reconstructing color images of astronomical objects using black and white spectroscopic emulsions

A color photograph of the peculiar elliptical galaxy NGC 5128 (Centaurus A) has been reconstructed from three Kodak 103a emulsion type photographs by projecting positives of the three B&W plates through appropriate filters onto a conventional color film. The resulting photograph shows color balance and latitude characteristics superior to color photographs of similar astronomical objects made with commercially available conventional color film. Similar results have been obtained for color reconstructed photographs of the Large and Small Magellanic Clouds. These and other results suggest that these projection-reconstruction techniques can be used to obtain high-quality color photographs of astronomical objects which overcome many of the problems associated with the use of conventional color film for the long exposures required in astronomy.

Dufour, R. I.

Electrography and astronomical applications

A review is presented of a conference on electrographic detectors in astronomy announced in IAA, issue 9, p. 1377, A75-23926. Different electrographic camera designs are described, and schematic diagrams of various image intensifiers (Lallemand, Kron, and Spectracon) are presented.

Martins, D. H.