Search Publications

The Metal-enriched Thermal Composite Supernova Remnant Kesteven 41 (G337.8-0.1) in a Molecular Environment
DOI: 10.1088/0004-637X/799/1/103 Bibcode: 2015ApJ...799..103Z

Zhou, Ping; Su, Yang; Zhou, Xin +3 more

The physical nature of thermal composite supernova remnants (SNRs) remains controversial. We have revisited the archival XMM-Newton and Chandra data of the thermal composite SNR Kesteven 41 (Kes 41 or G337.8-0.1) and performed a millimeter observation toward this source in the 12CO, 13CO, and C18O lines. The X-ray …

2015 The Astrophysical Journal
XMM-Newton 26
The SLUGGS survey: multipopulation dynamical modelling of the elliptical galaxy NGC 1407 from stars and globular clusters
DOI: 10.1093/mnras/stv831 Bibcode: 2015MNRAS.450.3345P

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P. +7 more

We perform in-depth dynamical modelling of the luminous and dark matter (DM) content of the elliptical galaxy NGC 1407. Our strategy consists of solving the spherical Jeans equations for three independent dynamical tracers: stars, blue globular clusters (GCs) and red GCs in a self-consistent manner. We adopt a maximum-likelihood Markov Chain Monte…

2015 Monthly Notices of the Royal Astronomical Society
eHST 26
Evaluating the Morphology of the Local Interstellar Medium: Using New Data to Distinguish between Multiple Discrete Clouds and a Continuous Medium
DOI: 10.1088/0004-637X/812/2/125 Bibcode: 2015ApJ...812..125R

Redfield, Seth; Linsky, Jeffrey L.

Ultraviolet and optical spectra of interstellar gas along the lines of sight to nearby stars have been interpreted by Redfield & Linsky and previous studies as a set of discrete warm, partially ionized clouds each with a different flow vector, temperature, and metal depletion. Recently, Gry & Jenkins proposed a fundamentally different mode…

2015 The Astrophysical Journal
eHST 26
First Infrared-Based Implications for the Dust Attenuation and Star Formation of Typical Lyα Emitters
DOI: 10.1088/2041-8205/800/2/L29 Bibcode: 2015ApJ...800L..29K

Ouchi, Masami; Shimasaku, Kazuhiro; Nakajima, Kimihiko +1 more

By stacking publicly available deep Spitzer/MIPS 24 µm and Herschel/PACS images for 213 z≃ 2.18 Lyα Emitters (LAEs) in GOODS-South, we obtain a strong upper limit to the IR luminosity of typical LAEs and discuss their attenuation curve for the first time. The 3σ upper limit LTIR = 1.1× {{10}10} {{L}⊙ …

2015 The Astrophysical Journal
Herschel eHST 26
Testing the inversion of asteroids' Gaia photometry combined with ground-based observations
DOI: 10.1093/mnras/stv631 Bibcode: 2015MNRAS.450..333S

Tanga, P.; Cellino, A.; Bartczak, P. +2 more

We investigated the reliability of the genetic algorithm which will be used to invert the photometric measurements of asteroids collected by the European Space Agency Gaia mission. To do that, we performed several sets of simulations for 10 000 asteroids having different spin axis orientations, rotational periods and shapes. The observational epoc…

2015 Monthly Notices of the Royal Astronomical Society
Gaia 26
Cosmological tests of modified gravity: Constraints on F (R ) theories from the galaxy clustering ratio
DOI: 10.1103/PhysRevD.91.103503 Bibcode: 2015PhRvD..91j3503B

Brax, Philippe; Marinoni, Christian; Bel, Julien +1 more

The clustering ratio η , a large-scale structure observable originally designed to constrain the shape of the power spectrum of matter density fluctuations, is shown to provide a sensitive probe of the nature of gravity in the cosmological regime. We apply this analysis to F (R ) theories of gravity using the luminous red galaxy sample extracted f…

2015 Physical Review D
Planck 26
Surface charging and electrostatic dust acceleration at the nucleus of comet 67P during periods of low activity
DOI: 10.1016/j.pss.2015.08.008 Bibcode: 2015P&SS..119...24N

Coates, A. J.; Jones, G. H.; Roussos, E. +2 more

We have investigated through simulation the electrostatic charging of the nucleus of Comet 67P/Churyumov-Gerasimenko during periods of weak outgassing activity. Specifically, we have modeled the surface potential and electric field at the surface of the nucleus during the initial Rosetta rendezvous at 3.5 AU and the release of the Philae lander at…

2015 Planetary and Space Science
Rosetta 26
The Absolute Age of the Globular Cluster M15 Using Near-infrared Adaptive Optics Images from PISCES/LBT.
DOI: 10.1088/0004-637X/812/1/25 Bibcode: 2015ApJ...812...25M

Boutsia, K.; Massari, D.; Arcidiacono, C. +26 more

We present deep near-infrared J, {K}{{s}} photometry of the old, metal-poor Galactic globular cluster M15 obtained with images collected with the LUCI1 and PISCES cameras available at the Large Binocular Telescope (LBT). We show how the use of First Light Adaptive Optics (FLAO) system coupled with the PISCES camera allows us to improve …

2015 The Astrophysical Journal
eHST 26
AKARI Observation of the Sub-degree Scale Fluctuation of the Near-infrared Background
DOI: 10.1088/0004-637X/807/2/140 Bibcode: 2015ApJ...807..140S

Lee, Hyung Mok; Lee, Myung Gyoon; Jeong, W. -S. +3 more

We report spatial fluctuation analysis of the sky brightness in the near-infrared from observations toward the north ecliptic pole (NEP) by the AKARI at 2.4 and 3.2 µm. As a follow-up study of our previous work on the Monitor field of AKARI, we used NEP deep survey data, which covered a circular area of about 0.4 square degrees, in order to …

2015 The Astrophysical Journal
AKARI 26
The far-ultraviolet main auroral emission at Jupiter - Part 1: Dawn-dusk brightness asymmetries
DOI: 10.5194/angeo-33-1203-2015 Bibcode: 2015AnGeo..33.1203B

Khurana, K. K.; Badman, S. V.; Bonfond, B. +6 more

The main auroral emission at Jupiter generally appears as a quasi-closed curtain centered around the magnetic pole. This auroral feature, which accounts for approximately half of the total power emitted by the aurorae in the ultraviolet range, is related to corotation enforcement currents in the middle magnetosphere. Early models for these current…

2015 Annales Geophysicae
eHST 26