Search Results - "Glass, I. S"

Towards stellar effective temperatures and diameters at 1 per cent accuracy for future surveys by Casagrande, L., Portinari, L., Glass, I. S., Laney, D., Silva Aguirre, V., Datson, J., Andersen, J., Nordström, B., Holmberg, J., Flynn, C., Asplund, M.

“…The apparent size of stars is a crucial benchmark for fundamental stellar properties such as effective temperatures, radii and surface gravities. While…”
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Long-term infrared photometry of Seyferts by Glass, I. S.

“…Long-term (up to 10 000 d) monitoring has been undertaken for 41 Seyferts in the near-infrared (1.25–3.45 μm). All but two showed variability, with amplitudes…”
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Semiregular variables in the solar neighbourhood by Glass, I. S., Van Leeuwen, F.

“…Period–luminosity sequences have been shown to exist among the semiregular variables (SRVs) in the Magellanic Clouds, the bulge of the Milky Way galaxy and…”
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The Nature of the Nuclear H2O Masers of NGC 1068: Reverberation and Evidence for a Rotating Disk Geometry by Gallimore, J. F, Henkel, C, Baum, S. A, Glass, I. S, Claussen, M. J, Prieto, M. A, Von Kap-herr, A

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Infrared stellar populations in the central parts of the Milky Way galaxy by Loon, Jacco Th. van, Gilmore, G. F., Omont, A., Blommaert, J. A. D. L., Glass, I. S., Messineo, M., Schuller, F., Schultheis, M., Yamamura, I., Zhao, H. S.

“…ABSTRACT Near‐ and mid‐IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10° (1.4 kpc) of the Milky…”
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The calibrating stars of the Mira P—L relation by Glass, I. S., Evans, T. Lloyd

“…Improved light curves extracted from the MACHO data base are used to discuss the periods and amplitudes of the calibrating stars of the Mira P–L relations…”
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Large-amplitude variables near the Galactic Centre by Glass, I. S., Matsumoto, S., Carter, B. S., Sekiguchi, K.

“…Abstract We report here the results of a 4-yr K-band (2.2 μm) survey for large-amplitude variable stars in a area centred on the Galactic Centre. A total of…”
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Period—magnitude relations for M giants in Baade's Window NGC 6522 by Glass, I. S., Schultheis, M.

“…A large and complete sample of stars with K < 9.75 in the NGC 6522 Baade's Window towards the Galactic bulge is examined using light curves extracted from…”
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Variability of Seyfert galaxies in the near-infrared — II. The unusual starburst Seyfert NGC 7469 by Glass, I. S.

“…The bright Seyfert 1 and starburst galaxy NGC 7469 has been monitored at JHKL for 13 yr. Its variations have been small, amounting to less than 0.3 mag, except…”
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Asymptotic giant branch variables in Baade's Windows by Schultheis, M., Glass, I.S.

“…In this work, a sample of luminous M-type giants in the Baade's Windows towards the inner Galactic bulge is investigated in the near-infrared. The ISOGAL…”
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A period–luminosity–colour relation for Mira variables by Feast, M. W., Glass, I. S., Whitelock, P. A., Catchpole, R. M.

“…Time-averaged J, H, K and mbol magnitudes are given for 29 O-rich and 20 C-rich Mira variables in the Large Magellanic Cloud. PL and PC relations are derived…”
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Mass-losing Semiregular Variable Stars in Baade's Windows by Alard, C, Blommaert, J. A. D. L, Cesarsky, C, Epchtein, N, Felli, M, Fouque, P, Ganesh, S, Genzel, R, Gilmore, G, Glass, I. S, Habing, H, Omont, A, Perault, M, Price, S, Robin, A, Schultheis, M, Simon, G, van Loon, J. Th, Alcock, C, Allsman, R. A, Alves, D. R, Axelrod, T. S, Becker, A. C, Bennett, D. P, Cook, K. H, Drake, A. J, Freeman, K. C, Geha, M, Griest, K, Lehner, M. J, Marshall, S. L, Minniti, D, Nelson, C, Peterson, B. A, Popowski, P, Pratt, M. R, Quinn, P. J, Sutherland, W, Tomaney, A. B, Vandehei, T, Welch, D. L

“…By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been…”
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Variability of Seyfert galaxies in the near-infrared. I - An outburst in NGC 2992 by Glass, I S

“…The IR light curve of the Seyfert 1.9 galaxy NGC 2992 shows a strong outburst between JD 244 7243 and 244 8734 of total energy 6 x 10 exp 43 J and having an…”
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ISOGAL survey of Baade's Windows in the mid-infrared by Glass, I. S., Ganesh, S., Alard, C., Blommaert, J. A. D. L., Gilmore, G., Lloyd Evans, T., Omont, A., Schultheis, M., Simon, G.

“…The ISOGAL mid-infrared survey of areas close to the Galactic plane aims to determine the stellar content of those areas, and its possible bearing on the…”
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Mid-infrared period–magnitude relations for AGB stars by Glass, I. S., Schultheis, M., Blommaert, J. A. D. L., Sahai, R., Stute, M., Uttenthaler, S.

“…Asymptotic giant branch (AGB) variables are found to obey period–luminosity relations in the mid-infrared (mid-IR) similar to those seen at KS (2.14 μm), even…”
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The variability of Magellanic cluster infrared stars by Nishida, S., Tanabé, T., Nakada, Y., Matsumoto, S., Sekiguchi, K., Glass, I. S.

“…We report on the light variations of the infrared stars that were discovered recently in the Magellanic clusters NGC 419, 1783 and 1978. Their periods, of 528,…”
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Infrared variability of the Seyfert galaxy NGC 3783 by GLASS, I. S

“…The results of about 15 years of monitoring of the variable Seyfert 1 galaxy NGC 3783 in the infrared are presented. The spectrum of the variable component…”
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Duration of the superwind phase of asymptotic giant branch stars by Tanabé, T, Nishida, S, Matsumoto, S, Onaka, T, Nakada, Y, Soyano, T, Ono, T, Sekiguchi, K, Glass, I. S000

“…The discovery of two infrared stars in Magellanic Cloud globular clusters that are undergoing a period of intense mass loss is discussed. Observations confirm…”
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Variability studies of Seyfert galaxies – I. Broad-band optical photometry by Winkler, H., Glass, I. S., van Wyk, F., Marang, F., Jones, J. H. Spencer, Buckley, D. A. H., Sekiguchi, K.

“…We present the results of a four-year campaign to monitor the variations of 35 southern Seyfert galaxies, using $UBV(RI)_\text C multi-aperture photometry…”
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Luminous variables in the Quintuplet cluster by Glass, I. S., Matsumoto, S., Carter, B. S., Sekiguchi, K.

“…We report observations of variability amongst the stars of the ‘Quintuplet’ cluster located about 30 pc in projection from the centre of the Galaxy. Two of the…”
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