The narrow X-ray tail and double Hα tails of ESO 137-002 in A3627

Zhang, B.; Sun, M.; Ji, L.; Sarazin, C.; Lin, X. B.; Nulsen, P. E. J.; Roediger, E.; Donahue, M.; Forman, W.; Jones, C.; Voit, G. M.; Kong, X.

doi:10.1088/0004-637x/777/2/122

Observationally-motivated analysis of simulated galaxies (2014)
Presentation / Conference Contribution
Gibson, B. K., MacFarlane, B. A., & Miranda, M. S. Observationally-motivated analysis of simulated galaxies. Presented at Proceedings of Science

© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. The spatial and temporal relationships between stellar age, kinematics, and chemistry are a fundamental tool for uncovering the p... Read More about Observationally-motivated analysis of simulated galaxies.

Cloud angular momentum and effective viscosity in global SPH simulations with feedback (2014)
Journal Article
Williamson, D. J., Thacker, R. J., Wurster, J., & Gibson, B. K. (2014). Cloud angular momentum and effective viscosity in global SPH simulations with feedback. Monthly notices of the Royal Astronomical Society, 442(4), 3674-3685. https://doi.org/10.1093/mnras/stu1121

We examine simulations of isolated galaxies to analyse the effects of localized feedback on the formation and evolution of molecular clouds. Feedback contributes to turbulence and the destruction of clouds, leading to a population of clouds that is y... Read More about Cloud angular momentum and effective viscosity in global SPH simulations with feedback.

Impact of the uncertainty in α-captures on 22Ne on the weak s-process in massive stars (2014)
Presentation / Conference Contribution
Nishimura, N., Hirschi, R., Pignatari, M., Herwig, F., Beard, M., Imbriani, G., Görres, J., Deboer, R. J., & Wiescher, M. Impact of the uncertainty in α-captures on 22Ne on the weak s-process in massive stars. Presented at ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2013: Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG12), Tsukuba, Japan

Massive stars at solar metallicity contribute to the production of heavy elements with atomic masses between A = 60 and A = 90 via the so-called weak s-process (which takes place during core He and shell C burning phases). Furthermore, recent studies... Read More about Impact of the uncertainty in α-captures on 22Ne on the weak s-process in massive stars.

The VMC ESO Public Survey (2013)
Journal Article
Cioni, M.-R. L., Anders, P., Bagheri, G., Bekki, K., Clementini, G., Emerson, J., Evans, C. J., For, B.-Q., De Grijs, R., Gibson, B. K., Girardi, L., Groenewegen, M. A. T., Guandalini, R., Gullieuszik, M., Ivanov, V. D., Kamath, D., Marconi, M., Marquette, J.-B., Miszalski, B., Moore, B., …Zaggia, S. (2013). The VMC ESO Public Survey. The Messenger, 23-25

The VISTA near-infrared YJKs survey of the Magellanic Clouds system (VMC) has entered its core phase: about 50% of the observations across the Large and Small Magellanic Clouds (LMC, SMC), the Magellanic Bridge and Stream have already been secured an... Read More about The VMC ESO Public Survey.

Some noteworthy alternating trilinear forms (2013)
Journal Article
Draisma, J., & Shaw, R. (2014). Some noteworthy alternating trilinear forms. Journal of Geometry, 105(1), 167-176. https://doi.org/10.1007/s00022-013-0202-2

Given an alternating trilinear form T ∈ Alt(×3Vn) on Vn =V(n,F) let LT denote the set of T-singular lines in PG(n-1)=PVn, consisting that is of those lines 〈a,b〉 of PG(n-1) such that T(a, b, x) = 0 for all x ∈ Vn. Amongst the immense profusion of d... Read More about Some noteworthy alternating trilinear forms.

Leggett-Garg inequalities (2013)
Journal Article
Emary, C., Lambert, N., & Nori, F. (2014). Leggett-Garg inequalities. Reports on progress in physics, 77(1), Article 016001. https://doi.org/10.1088/0034-4885/77/1/016001

In contrast to the spatial Bell’s inequalities which probe entanglement between spatially-separated systems, the Leggett-Garg inequalities test the correlations of a single system measured at different times. Violation of a genuine Leggett-Garg test... Read More about Leggett-Garg inequalities.

Numerical simulations of bubble-induced star formation in dwarf irregular galaxies with a novel stellar feedback scheme (2013)
Journal Article
Kawata, D., Gibson, B. K., Barnes, D. J., Grand, R. J., & Rahimi, A. (2014). Numerical simulations of bubble-induced star formation in dwarf irregular galaxies with a novel stellar feedback scheme. Monthly notices of the Royal Astronomical Society, 438(2), 1208-1222. https://doi.org/10.1093/mnras/stt2267

To study the star formation and feedback mechanism, we simulate the evolution of an isolated dwarf irregular galaxy (dIrr) in a fixed dark matter halo, similar in size to Wolf–Lundmark–Melotte, using a new stellar feedback scheme. We use the new vers... Read More about Numerical simulations of bubble-induced star formation in dwarf irregular galaxies with a novel stellar feedback scheme.

Galaxy and mass assembly (GAMA): The large-scale structure of galaxies and comparison to mock universes (2013)
Journal Article
Alpaslan, M., Robotham, A. S. G., Driver, S., Norberg, P., Baldry, I., Bauer, A. E., Bland-Hawthorn, J., Brown, M., Cluver, M., Colless, M., Foster, C., Hopkins, A., Van kampen, E., Kelvin, L., Lara-Lopez, M. A., Liske, J., Lopez-Sanchez, A. R., Loveday, J., Mcnaught-Roberts, T., Merson, A., & Pimbblet, K. (2014). Galaxy and mass assembly (GAMA): The large-scale structure of galaxies and comparison to mock universes. Monthly notices of the Royal Astronomical Society, 438(1), 177-194. https://doi.org/10.1093/mnras/stt2136

From a volume-limited sample of 45 542 galaxies and 6000 groups with z ≤ 0.213, we use an adapted minimal spanning tree algorithm to identify and classify large-scale structures within the Galaxy And Mass Assembly (GAMA) survey. Using galaxy groups,... Read More about Galaxy and mass assembly (GAMA): The large-scale structure of galaxies and comparison to mock universes.

Phase mixing due to the Galactic potential: steps in the position and velocity distributions of popped star clusters (2013)
Journal Article
Candlish, G. N., Smith, R., Fellhauer, M., Gibson, B. K., Kroupa, P., & Assmann, P. (2014). Phase mixing due to the Galactic potential: steps in the position and velocity distributions of popped star clusters. Monthly notices of the Royal Astronomical Society, 437(4), 3702-3717. https://doi.org/10.1093/mnras/stt2166

As star clusters are expected to form with low star formation efficiencies, the gas in the cluster is expelled quickly and early in their development: the star cluster ‘pops’. This leads to an unbound stellar system, evolving in the Galactic potentia... Read More about Phase mixing due to the Galactic potential: steps in the position and velocity distributions of popped star clusters.

A fragment method for systematic improvement of anharmonic adsorbate vibrational frequencies: Acetylene on Cu(001) (2013)
Journal Article
Chulkov, S. K., & Benoit, D. M. (2013). A fragment method for systematic improvement of anharmonic adsorbate vibrational frequencies: Acetylene on Cu(001). The Journal of chemical physics, 139(21), Article 214704. https://doi.org/10.1063/1.4829461

We suggest a novel method for systematic improvement of anharmonic adsorbate frequencies based on a fragment approach. The calculations are carried out by considering the adsorbed molecule separately and computing an energy correction using high-leve... Read More about A fragment method for systematic improvement of anharmonic adsorbate vibrational frequencies: Acetylene on Cu(001).

Angular distribution in the neutron-induced fission of actinides (2013)
Journal Article
Leong, L., Tassan-Got, L., Tarrio, D., Audouin, L., Paradela, C., Duran, I., Le Naour, C., Altstadt, S., Andrzejewsky, J., Barbagallo, M., Bécares, V., Bečvář, F., Belloni, F., Berthoumieux, E., Billowes, J., Boccone, V., Bosnar, D., Brugger, M., Calvino, F., Calviani, M., …González, R. (2013). Angular distribution in the neutron-induced fission of actinides. EPJ Web of Conferences, 62, 08003. https://doi.org/10.1051/epjconf/20136208003

Above 1 MeV of incident neutron energy the fission fragment angular distribution (FFAD) has generally a strong anisotropic behavior due to the combination of the incident orbital momentum and the intrinsic spin of the fissioning nucleus. This effect... Read More about Angular distribution in the neutron-induced fission of actinides.

Measurement of the MACS of Ta 181 (n, γ) at kT=30 keV as a test of a method for Maxwellian neutron spectra generation (2013)
Journal Article
Praena, J., Mastinu, P., Pignatari, M., Quesada, J., García-López, J., Lozano, M., Dzysiuk, N., Capote, R., & Martín-Hernández, G. (2013). Measurement of the MACS of Ta 181 (n, γ) at kT=30 keV as a test of a method for Maxwellian neutron spectra generation. Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 727, 1-6. https://doi.org/10.1016/j.nima.2013.05.151

Measurement of the Maxwellian-Averaged Cross-Section (MACS) of the Ta(n,γ)181 reaction at kT=30 keV by the activation technique using an innovative method for the generation of Maxwellian neutron spectra is presented. The method is based on the shapi... Read More about Measurement of the MACS of Ta 181 (n, γ) at kT=30 keV as a test of a method for Maxwellian neutron spectra generation.

Environments and morphologies of red sequence galaxies with residual star formation in massive clusters (2013)
Journal Article
Crossett, J. P., Pimbblet, K. A., Stott, J. P., & Jones, D. H. (2014). Environments and morphologies of red sequence galaxies with residual star formation in massive clusters. Monthly notices of the Royal Astronomical Society, 437(3), 2521-2530. https://doi.org/10.1093/mnras/stt2065

We present a photometric investigation into recent star formation in galaxy clusters at z ∼ 0.1. We use spectral energy distribution templates to quantify recent star formation in large Xray-selected clusters from the LARCS survey using matched GALEX... Read More about Environments and morphologies of red sequence galaxies with residual star formation in massive clusters.

Phase mixing of popped star clusters (2013)
Presentation / Conference Contribution
Candlish, G. N., Smith, R., Fellhauer, M., Gibson, B. K., Kroupa, P., & Assmann, P. (2013, November). Phase mixing of popped star clusters. Presented at XIV Latin American Regional IAU Meeting

As star clusters are expected to form with low star formation efficiencies, the gas in the cluster is expelled quickly and early in their development: the star cluster pops. This leads to an unbound stellar system. Previous N-body simulations have de... Read More about Phase mixing of popped star clusters.

Water-in-water emulsions based on incompatible polymers and stabilized by triblock copolymers-templated polymersomes (2013)
Journal Article
Buzza, D. M. A., Fletcher, P. D. I., Georgiou, T. K., & Ghasdian, N. (2013). Water-in-water emulsions based on incompatible polymers and stabilized by triblock copolymers-templated polymersomes. Langmuir : the ACS journal of surfaces and colloids, 29(48), 14804-14814. https://doi.org/10.1021/la403356j

Aqueous solutions containing a mixture of polyethylene glycol (PEG) and dextran homopolymers form an aqueous two-phase system which can be emulsified to give a water-in-water emulsion. We show how these emulsions can be stabilized using triblock poly... Read More about Water-in-water emulsions based on incompatible polymers and stabilized by triblock copolymers-templated polymersomes.

Two-magnon bound state causes ultrafast thermally induced magnetisation switching (2013)
Journal Article
Barker, J., Atxitia, U., Hovorka, O., Ostler, T. A., Chubykalo-Fesenko, O., & Chantrell, R. W. (2013). Two-magnon bound state causes ultrafast thermally induced magnetisation switching. Scientific reports, 3, Article 3262. https://doi.org/10.1038/srep03262

There has been much interest recently in the discovery of thermally induced magnetisation switching using femtosecond laser excitation, where a ferrimagnetic system can be switched deterministically without an applied magnetic field. Experimental res... Read More about Two-magnon bound state causes ultrafast thermally induced magnetisation switching.

The [α/Fe] ratios of very metal-poor stars within the integrated galactic initial mass function theory (2013)
Journal Article
Recchi, S., Calura, F., Kroupa, P., & Gibson, B. K. (2014). The [α/Fe] ratios of very metal-poor stars within the integrated galactic initial mass function theory. Monthly notices of the Royal Astronomical Society, 437(1), 994-1008. https://doi.org/10.1093/mnras/stt1971

The aim of this paper is to quantify the amplitude of the predicted plateau in [α/Fe] ratios associated with the most metal-poor stars of a galaxy. We assume that the initial mass function (IMF) in galaxies is steeper if the star formation rate (SFR)... Read More about The [α/Fe] ratios of very metal-poor stars within the integrated galactic initial mass function theory.

Diffuse interstellar band at 8620 Å in RAVE : a new method for detecting the diffuse interstellar band in spectra of cool stars (2013)
Journal Article
Bland-Hawthorn, J., Kos, J., Zwitter, T., Grebel, E. K., Bienayme, O., Binney, J., Freeman, K. C., Gibson, B. K., Gilmore, G., Kordopatis, G., Navarro, J. F., Parker, Q., Reid, W. A., Seabroke, G., Siebert, A., Siviero, A., Steinmetz, M., Watson, F., & Wyse, R. F. G. (2013). Diffuse interstellar band at 8620 Å in RAVE : a new method for detecting the diffuse interstellar band in spectra of cool stars. The Astrophysical journal, 778(2), 86. https://doi.org/10.1088/0004-637x/778/2/86

Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar lines are rarely blended with stellar ones. The need for hot stars is a strong limitation in the number of sightlines we can observe and their distribu... Read More about Diffuse interstellar band at 8620 Å in RAVE : a new method for detecting the diffuse interstellar band in spectra of cool stars.

Relics of ancient post-AGB stars in a primitive meteorite (2013)
Journal Article
Jadhav, M., Pignatari, M., Herwig, F., Zinner, E., Gallino, R., & Huss, G. R. (2013). Relics of ancient post-AGB stars in a primitive meteorite. Astrophysical journal. Letters, 777(2), L27. https://doi.org/10.1088/2041-8205/777/2/l27

Graphite is one of the many presolar circumstellar condensate species found in primitive meteorites. While the isotopic compositions of low-density graphite grains indicate an origin in core-collapse supernovae, some high-density grains have extreme... Read More about Relics of ancient post-AGB stars in a primitive meteorite.

The narrow X-ray tail and double Hα tails of ESO 137-002 in A3627 (2013)
Journal Article
Zhang, B., Sun, M., Ji, L., Sarazin, C., Lin, X. B., Nulsen, P. E. J., Roediger, E., Donahue, M., Forman, W., Jones, C., Voit, G. M., & Kong, X. (2013). The narrow X-ray tail and double Hα tails of ESO 137-002 in A3627. The Astrophysical journal, 777(2), Article 122. https://doi.org/10.1088/0004-637x/777/2/122

We present the analysis of a deep Chandra observation of a ~2 L * late-type galaxy, ESO 137-002, in the closest rich cluster A3627. The Chandra data reveal a long (gsim40 kpc) and narrow tail with a nearly constant width (~3 kpc) to the southeast of... Read More about The narrow X-ray tail and double Hα tails of ESO 137-002 in A3627.

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