Outputs (286)

Stripped elliptical galaxies as probes of ICM physics: I. Tails, wakes, and flow patterns in and around stripped ellipticals (2015)
Journal Article
Roediger, E., Kraft, R. P., Nulsen, P. E. J., Forman, W. R., Machacek, M., Randall, S., Jones, C., Churazov, E., & Kokotanekova, R. (2015). Stripped elliptical galaxies as probes of ICM physics: I. Tails, wakes, and flow patterns in and around stripped ellipticals. The Astrophysical journal, 806(1), Article ARTN 103. https://doi.org/10.1088/0004-637X/806/1/103

Elliptical cluster galaxies are progressively stripped of their atmospheres due to their motion through the intra-cluster medium (ICM). Deep X-ray observations reveal the fine-structure of the galaxy's remnant atmosphere and its gas tail and wake. Th... Read More about Stripped elliptical galaxies as probes of ICM physics: I. Tails, wakes, and flow patterns in and around stripped ellipticals.

Stripped elliptical galaxies as probes of ICM physics: II. Stirred, but mixed? Viscous and inviscid gas stripping of the Virgo elliptical M89 (2015)
Journal Article
Roediger, E., Kraft, R. P., Nulsen, P. E. J., Forman, W. R., Machacek, M., Randall, S., Jones, C., Churazov, E., & Kokotanekova, R. (2015). Stripped elliptical galaxies as probes of ICM physics: II. Stirred, but mixed? Viscous and inviscid gas stripping of the Virgo elliptical M89. The Astrophysical journal, 806(1), 104. https://doi.org/10.1088/0004-637X/806/1/104

Elliptical galaxies moving through the intra-cluster medium (ICM) are progressively stripped of their gaseous atmospheres. X-ray observations reveal the structure of galactic tails, wakes, and the interface between the galactic gas and the ICM. This... Read More about Stripped elliptical galaxies as probes of ICM physics: II. Stirred, but mixed? Viscous and inviscid gas stripping of the Virgo elliptical M89.

An alternative methodology to assess the quality of empirical potentials for small gold clusters (2015)
Journal Article
Mancera, L. A., & Benoit, D. M. (2015). An alternative methodology to assess the quality of empirical potentials for small gold clusters. Computational and Theoretical Chemistry, 1067(September), 24-32. https://doi.org/10.1016/j.comptc.2015.05.026

We present a methodology based on local comparisons of potential energy surfaces (PES) in order to assess the quality of empirical potentials. We compare five typical empirical potentials using a criterion that shows which of these potentials resembl... Read More about An alternative methodology to assess the quality of empirical potentials for small gold clusters.

On the abundance of extreme voids (2015)
Journal Article
Chongchitnan, S. (2015). On the abundance of extreme voids. Journal of cosmology and astroparticle physics, May(05), 062-062. https://doi.org/10.1088/1475-7516/2015/05/062

Cosmic voids have been shown to be an effective probe of cosmology, complementary to galaxy clusters. In this work, we present a simple theoretical framework for predicting of the size of the largest voids expected within a given redshift and volume.... Read More about On the abundance of extreme voids.

Understanding of matrix embedding: a theoretical spectroscopic study of CO interacting with Ar clusters, surfaces and matrices (2015)
Journal Article
Mahjoubi, K., Benoit, D. M., Jaidane, N.-E., Al-Mogren, M. M., & Hochlaf, M. (2015). Understanding of matrix embedding: a theoretical spectroscopic study of CO interacting with Ar clusters, surfaces and matrices. Physical chemistry chemical physics : PCCP, 17(26), 17159-17168. https://doi.org/10.1039/c5cp01672j

Through benchmark studies, we explore the performance of PBE density functional theory, with and without Grimme's dispersion correction (DFT-D3), in predicting spectroscopic properties for molecules interacting with rare gas matrices. Here, a periodi... Read More about Understanding of matrix embedding: a theoretical spectroscopic study of CO interacting with Ar clusters, surfaces and matrices.

Tracking Cluster Debris (TraCD) – I. Dissolution of clusters and searching for the solar cradle (2015)
Journal Article
Moyano Loyola, G. R., Flynn, C., Hurley, J. R., & Gibson, B. K. (2015). Tracking Cluster Debris (TraCD) – I. Dissolution of clusters and searching for the solar cradle. Monthly notices of the Royal Astronomical Society, 449(4), 4443-4457. https://doi.org/10.1093/mnras/stv550

The capability to reconstruct dissolved stellar systems in dynamical and chemical space is a key factor in improving our understanding of the evolution of the Milky Way. Here we concentrate on the dynamical aspect and given that a significant portion... Read More about Tracking Cluster Debris (TraCD) – I. Dissolution of clusters and searching for the solar cradle.

The nature and role of the gold-krypton interactions in small neutral gold clusters (2015)
Journal Article
Mancera, L. A., & Benoit, D. M. (2015). The nature and role of the gold-krypton interactions in small neutral gold clusters. The journal of physical chemistry. A, 119(12), 3075-3088. https://doi.org/10.1021/jp513021q

© 2015 American Chemical Society. We investigate the nature and role of krypton embedding in small neutral gold clusters. For some of these clusters, we observe a particular site-dependent character of the Kr binding that does not completely follow t... Read More about The nature and role of the gold-krypton interactions in small neutral gold clusters.

Simple and accurate modelling of the gravitational potential produced by thick and thin exponential discs (2015)
Journal Article
Smith, R., Flynn, C., Candlish, G. N., Fellhauer, M., & Gibson, B. K. (2015). Simple and accurate modelling of the gravitational potential produced by thick and thin exponential discs. Monthly notices of the Royal Astronomical Society, 448(3), 2934-2940. https://doi.org/10.1093/mnras/stv228

We present accurate models of the gravitational potential produced by a radially exponential disc mass distribution. The models are produced by combining three separate Miyamoto–Nagai discs. Such models have been used previously to model the disc of... Read More about Simple and accurate modelling of the gravitational potential produced by thick and thin exponential discs.

The imprints of the Galactic Bar on the Thick Disk with RAVE (2015)
Journal Article
Antoja, T., Monari, G., Helmi, A., Bienaymé, O., Bland-Hawthorn, J., Famaey, B., Gibson, B. K., Grebel, E. K., Kordopatis, G., Munari, U., Navarro, J., Parker, Q., Reid, W. A., Seabroke, G., Antoja, T., Steinmetz, M., & Zwitter, T. (2015). The imprints of the Galactic Bar on the Thick Disk with RAVE. Astrophysical journal. Letters, 800(2), L32. https://doi.org/10.1088/2041-8205/800/2/l32

We study the kinematics of a local sample of stars, located within a cylinder of 500 pc radius centered on the Sun, in the RAVE data set. We find clear asymmetries in the v R v∞ velocity distributions of thin and thick disk stars: there are more sta... Read More about The imprints of the Galactic Bar on the Thick Disk with RAVE.

The influence of red spiral galaxies on the shape of the local K-band luminosity function (2015)
Journal Article
Bonne, N. J., Brown, M. J. I., Jones, H., & Pimbblet, K. A. (2015). The influence of red spiral galaxies on the shape of the local K-band luminosity function. The Astrophysical journal, 799(2), Article ARTN 160. https://doi.org/10.1088/0004-637x/799/2/160

We have determined K-band luminosity functions for 13,325 local universe galaxies as a function of morphology and color (for Ktot ≤ 10.75). Our sample is drawn from the Two Micron All Sky Survey Extended Source Catalog, with all sample galaxies havin... Read More about The influence of red spiral galaxies on the shape of the local K-band luminosity function.

Sulfur isotopic compositions of submicrometer SiC grains from the Murchison meteorite (2015)
Journal Article
Xu, Y., Zinner, E., Gallino, R., Heger, A., Pignatari, M., & Lin, Y. (2015). Sulfur isotopic compositions of submicrometer SiC grains from the Murchison meteorite. The Astrophysical journal, 799(2), 156. https://doi.org/10.1088/0004-637x/799/2/156

We report C, Si, N, S, Mg-Al, and Ca-Ti isotopic compositions of presolar silicon carbide (SiC) grains from the SiC-rich KJE size fraction (0.5-0.8 μm) of the Murchison meteorite. One thousand one hundred thirteen SiC grains were identified based on... Read More about Sulfur isotopic compositions of submicrometer SiC grains from the Murchison meteorite.

The rich are different: evidence from the RAVE survey for stellar radial migration (2015)
Journal Article
Kordopatis, G., Binney, J., Gilmore, G., Wyse, R. F. G., Belokurov, V., McMillan, P. J., Hatfield, P., Grebel, E. K., Steinmetz, M., Navarro, J. F., Seabroke, G., Minchev, I., Chiappini, C., Bienaymé, O., Bland-Hawthorn, J., Freeman, K. C., Gibson, B. K., Helmi, A., Munari, U., Parker, Q., …Zwitter, T. (2015). The rich are different: evidence from the RAVE survey for stellar radial migration. Monthly notices of the Royal Astronomical Society, 447(4), 3526-3535. https://doi.org/10.1093/mnras/stu2726

Using the RAdial Velocity Experiment fourth data release (RAVE DR4), and a new metallicity calibration that will be also taken into account in the future RAVE DR5, we investigate the existence and the properties of super-solar metallicity stars ([M/H... Read More about The rich are different: evidence from the RAVE survey for stellar radial migration.

Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning (2015)
Journal Article
Jones, S., Hirschi, R., Pignatari, M., Heger, A., Georgy, C., Nishimura, N., Fryer, C., & Herwig, F. (2015). Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning. Monthly notices of the Royal Astronomical Society, 447(4), 3115-3129. https://doi.org/10.1093/mnras/stu2657

Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of massive star models computed by different groups each using their own codes, input physics choices and numerical approximations, however, lead to inco... Read More about Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning.

Characterizing the high-velocity stars of RAVE: the discovery of a metal-rich halo star born in the Galactic disc (2015)
Journal Article
Hawkins, K., Kordopatis, G., Gilmore, G., Masseron, T., Wyse, R. F. G., Ruchti, G., Bienaymé, O., Bland-Hawthorn, J., Boeche, C., Freeman, K., Gibson, B. K., Grebel, E. K., Helmi, A., Kunder, A., Munari, U., Navarro, J. F., Parker, Q. A., Reid, W. A., Scholz, R. D., Seabroke, G., …Zwitter, T. (2015). Characterizing the high-velocity stars of RAVE: the discovery of a metal-rich halo star born in the Galactic disc. Monthly notices of the Royal Astronomical Society, 447(2), 2046-2058. https://doi.org/10.1093/mnras/stu2574

© 2015 The Authors. We aim to characterize high-velocity (HiVel) stars in the solar vicinity both chemically and kinematically using the fourth data release of the RAdial Velocity Experiment (RAVE). We used a sample of 57HiVel starswith Galactic rest... Read More about Characterizing the high-velocity stars of RAVE: the discovery of a metal-rich halo star born in the Galactic disc.

Identification of globular cluster stars in RAVE data - I. Application to stellar parameter calibration (2015)
Journal Article
Anguiano, B., Zucker, D. B., Scholz, R. D., Grebel, E. K., Seabroke, G., Kunder, A., Binney, J., McMillan, P. J., Zwitter, T., Wyse, R., Kordopatis, G., Bienaymé, O., Bland-Hawthorn, J., Boeche, C., Freeman, K. C., Gibson, B. K., Gilmore, G., Munari, U., Navarro, J., Parker, Q., …Watson, F. (2015). Identification of globular cluster stars in RAVE data - I. Application to stellar parameter calibration. Monthly notices of the Royal Astronomical Society, 451(2), 1229-1246. https://doi.org/10.1093/mnras/stv800

We present the identification of potential members of nearby Galactic globular clusters using radial velocities from the RAdial Velocity Experiment Data Release 4 (RAVE-DR4) survey data base. Our identifications are based on three globular clusters –... Read More about Identification of globular cluster stars in RAVE data - I. Application to stellar parameter calibration.

The clustering and halo masses of star-forming galaxies at z<1 (2014)
Journal Article
Dolley, T., Brown, M. J. I., Weiner, B. J., Brodwin, M., Kochanek, C. S., Pimbblet, K. A., Palamara, D. P., Jannuzi, B. T., Dey, A., Atlee, D. W., & Beare, R. (2014). The clustering and halo masses of star-forming galaxies at z

We present clustering measurements and halo masses of star-forming galaxies at 0.2 < z < 1.0. After excluding active galactic nuclei (AGNs), we construct a sample of 22,553 24 μm sources selected from 8.42 deg2 of the Spitzer MIPS AGN and Galaxy Evol... Read More about The clustering and halo masses of star-forming galaxies at z<1.

New insights on Ba overabundance in open clusters : evidence for the intermediate neutron-capture process at play? (2014)
Journal Article
Mishenina, T., Pignatari, M., Carraro, G., Kovtyukh, V., Monaco, L., Korotin, S., Shereta, E., Yegorova, I., & Herwig, F. (2015). New insights on Ba overabundance in open clusters : evidence for the intermediate neutron-capture process at play?. Monthly notices of the Royal Astronomical Society, 446(4), 3651-3668. https://doi.org/10.1093/mnras/stu2337

Recently, an increasing number of studies were devoted to measure the abundances of neutron-capture elements heavier than iron in stars belonging to Galactic Open Clusters (OCs). OCs span a sizeable range in metallicity (−0.6 ≤ [Fe/H] ≤ +0.4), and th... Read More about New insights on Ba overabundance in open clusters : evidence for the intermediate neutron-capture process at play?.

An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set (2014)
Journal Article
Beare, R., Brown, M. J. I., & Pimbblet, K. (2014). An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set. The Astrophysical journal, 797(2), Article ARTN 104. https://doi.org/10.1088/0004-637x/797/2/104

We describe an accurate new method for determining absolute magnitudes, and hence also K-corrections, that is simpler than most previous methods, being based on a quadratic function of just one suitably chosen observed color. The method relies on the... Read More about An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set.

Spectroscopic signatures of extratidal stars around the globular clusters NGC 6656 (M 22), NGC 3201, and NGC 1851 from RAVE (2014)
Journal Article
Kunder, A., Bono, G., Piffl, T., Steinmetz, M., Grebel, E. K., Anguiano, B., Freeman, K., Kordopatis, G., Zwitter, T., Scholz, R., Gibson, B. K., Bland-Hawthorn, J., Seabroke, G., Boeche, C., Siebert, A., Wyse, R. F. G., Bienaymé, O., Navarro, J., Siviero, A., Minchev, I., …Helmi, A. (2014). Spectroscopic signatures of extratidal stars around the globular clusters NGC 6656 (M 22), NGC 3201, and NGC 1851 from RAVE. Astronomy and Astrophysics, 572, A30. https://doi.org/10.1051/0004-6361/201424113

© ESO, 2014. Context. Stellar population studies of globular clusters have suggested that the brightest clusters in the Galaxy might actually be the remnant nuclei of dwarf spheroidal galaxies. If the present Galactic globular clusters formed within... Read More about Spectroscopic signatures of extratidal stars around the globular clusters NGC 6656 (M 22), NGC 3201, and NGC 1851 from RAVE.

Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores (2014)
Journal Article
Merluzzi, P., Busarello, G., Haines, C. P., Mercurio, A., Okabe, N., Pimbblet, K. J., Dopita, M. A., Grado, A., Limatola, L., Bourdin, H., Mazzotta, P., Capaccioli, M., Napolitano, N. R., & Schipani, P. (2015). Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores. Monthly notices of the Royal Astronomical Society, 446(1), 803-822. https://doi.org/10.1093/mnras/stu2085

We present an overview of a multiwavelength survey of the Shapley Supercluster (SSC; z ∼ 0.05) covering a contiguous area of 260 h−2 70 Mpc² including the supercluster core. The project main aim is to quantify the influence of cluster-scale mass asse... Read More about Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores.