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Date: 2015
Subject Keyword: Galaxy: stellar content
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/355356
Description: The Galactic Archaeology with HERMES (GALAH) survey is a large high-resolution spectroscopic survey using the newly commissioned High Efficiency and Resolution Multi-Element Spectrograph (HERMES) on t ... More
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Reviewed: Reviewed
Date: 2014
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/304923
Description: Aims. We study the effects of moderate deviations from solar abundances upon the atmospheric structure and colours of typical Mira variables. Methods. We present two model series of dynamical opacity- ... More
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Reviewed: Reviewed
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271491
Description: We present the results of long-baseline optical interferometry observations using the Precision Astronomical Visual Observations (PAVO) beam combiner at the Center for High Angular Resolution Astronom ... More
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Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271584
Description: We present the first multiplicity-dedicated long-baseline optical interferometric survey of the Scorpius-Centaurus-Lupus-Crux association. We used the Sydney University Stellar Interferometer to under ... More
Reviewed: Reviewed
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271410
Description: We present interferometric observations of seven main-sequence and three giant stars with spectral types from B2 to F6 using the Precision Astronomical Visible Observations beam combiner at the Center ... More
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Authors: Ireland, M. J
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/226900
Description: Bispectrum phase, closure phase and their generalization to kernel phase are all independent of pupil-plane phase errors to first order. This property, when used with sparse aperture masking behind ad ... More
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/171003
Description: 21 page(s)
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/195560
Description: We present an analysis of the WISE photometric data for 829 stars in the Sco-Cen OB2 association, using the latest high-mass membership probabilities. We detect infrared excesses associated with 135 B ... More
Reviewed: Reviewed
Date: 2011
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/152389
Description: We present four model series of the CODEX dynamical opacity-sampling models of Mira variables with solar abundances, designed to have parameters similar to o Cet, R Leo and R Cas. We demonstrate that ... More
Reviewed: Reviewed
Date: 2011
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/143413
Description: We present a new high-mass membership of the nearby Sco OB2 association based on Hipparcos positions, proper motions and parallaxes, and radial velocities taken from the 2nd Catalogue of Radial Veloci ... More
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Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137689
Description: We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained with 30 minute sampli ... More
Reviewed: Reviewed
Authors: Chaplin, W. J | Appourchaux, T | Brown, T. M | Aguirre, V. S | Stevens, I. R | Suárez, J. C | Suran, M. D | Trampedach, R | Turck-Chièze, S | Uytterhoeven, K | Ventura, R | Wilson, P. A | Christensen-Dalsgaard, J | Gilliland, R. L | Kjeldsen, H | Borucki, W. J | Koch, D | Jenkins, J. M | Ballot, J | Basu, S | Bazot, M | Elsworth, Y | Bedding, T. R | Benomar, O | Bonanno, A | Brandão, I. M | Bruntt, H | Campante, T. L | Creevey, O. L | Mauro, M. P. Di | Doğan, G | Dreizler, S | García, R. A | Eggenberger, P | Esch, L | Fletcher, S. T | Frandsen, S | Gai, N | Gaulme, P | Handberg, R | Hekker, S | Howe, R | Huber, D | Houdek, G | Korzennik, S. G | Lebrun, J. C | Leccia, S | Martic, M | Mathur, S | Mosser, B | New, R | Quirion, P.-O | Régulo, C | Roxburgh, I. W | Karoff, C | Salabert, D | Schou, J | Sousa, S. G | Stello, D | Verner, G. A | Arentoft, T | Barban, C | Belkacem, K | Benatti, S | Biazzo, K | Metcalfe, T. S | Boumier, P | Bradley, P. A | Broomhall, A.-M | Buzasi, D. L | Claudi, R. U | Cunha, M. S | D'Antona, F | Deheuvels, S | Derekas, A | Hernández, A. García | Molenda-Żakowicz, J | Giampapa, M. S | Goupil, M. J | Gruberbauer, M | Guzik, J. A | Hale, S. J | Ireland, M. J | Kiss, L. L | Kitiashvili, I. N | Kolenberg, K | Korhonen, H | Monteiro, M. J. P. F. G | Kosovichev, A. G | Kupka, F | Lebreton, Y | Leroy, B | Ludwig, H.-G | Mathis, S | Michel, E | Miglio, A | Montalbán, J | Moya, A | Thompson, M. J | Noels, A | Noyes, R. W | Pallé, P. L | Piau, L | Preston, H. L | Cortés, T. Roca | Roth, M | Sato, K. H | Schmitt, J | Serenelli, A. M
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137906
Description: We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-nois ... More
Reviewed: Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/139375
Description: The growing interest in solar twins is motivated by the possibility of comparing them directly to the Sun. To carry on this kind of analysis, we need to know their physical characteristics with precis ... More
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Reviewed: Reviewed
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137633
Description: The mid-infrared properties of pre-planetary disks are sensitive to the temperature and flaring profiles of disks for the regions where planet formation is expected to occur. In order to constrain the ... More
Reviewed: Reviewed