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Mass Profile Decomposition of the Frontier Fields Cluster MACS J0416-2403: Insights on the Dark-matter Inner Profile
DOI: 10.3847/1538-4357/aa9845 Bibcode: 2017ApJ...851...81A

Grillo, C.; Rosati, P.; Lombardi, M. +8 more

We present a high-resolution dissection of the two-dimensional total mass distribution in the core of the Hubble Frontier Fields galaxy cluster MACS J0416.1-2403, at z = 0.396. We exploit HST/WFC3 near-IR (F160W) imaging, VLT/Multi Unit Spectroscopic Explorer spectroscopy, and Chandra data to separate the stellar, hot gas, and dark-matter mass com…

2017 The Astrophysical Journal
eHST 29
Polycyclic Aromatic Hydrocarbon Emission in Spitzer/IRS Maps. II. A Direct Link between Band Profiles and the Radiation Field Strength
DOI: 10.3847/1538-4357/aa5f54 Bibcode: 2017ApJ...837..129S

Peeters, E.; Stock, D. J.

We decompose the observed 7.7 µm polycyclic aromatic hydrocarbon (PAH) emission complexes in a large sample of over 7000 mid-infrared spectra of the interstellar medium using spectral cubes observed with the Spitzer/IRS-SL instrument. In order to fit the 7.7 µm PAH emission complex we invoke four Gaussian components, which are found to…

2017 The Astrophysical Journal
ISO 29
Probing the Anisotropy of the Milky Way Gaseous Halo-II: Sightline toward Mrk 509
DOI: 10.3847/1538-4357/836/2/243 Bibcode: 2017ApJ...836..243G

Krongold, Y.; Mathur, S.; Gupta, A.

Hot, million degree gas appears to pervade the Milky Way halo, containing a large fraction of the Galactic missing baryons. This circumgalactic medium (CGM) is probed effectively in X-rays, both in absorption and in emission. The CGM also appears to be anisotropic, so we have started a program to determine CGM properties along several sightlines b…

2017 The Astrophysical Journal
Suzaku XMM-Newton 29
The merger remnant NGC 3610 and its globular cluster system: a large-scale study
DOI: 10.1093/mnras/stw3390 Bibcode: 2017MNRAS.466.4259B

Bassino, Lilia P.; Caso, Juan P.

We present a photometric study of the prototype merger remnant NGC 3610 and its globular cluster (GC) system, based on new Gemini/GMOS and Advanced Camera for Surveys/Hubble Space Telescope archival images. Thanks to the large field of view of our GMOS data, larger than previous studies, we are able to detect a 'classical' bimodal GC colour distri…

2017 Monthly Notices of the Royal Astronomical Society
eHST 29
The First Simultaneous X-Ray/Radio Detection of the First Be/BH System MWC 656
DOI: 10.3847/2041-8213/835/2/L33 Bibcode: 2017ApJ...835L..33R

Iwasawa, K.; Migliari, S.; Marcote, B. +6 more

MWC 656 is the first known Be/black hole (BH) binary system. Be/BH binaries are important in the context of binary system evolution and sources of detectable gravitational waves because they are possible precursors of coalescing neutron star/BH binaries. X-ray observations conducted in 2013 revealed that MWC 656 is a quiescent high-mass X-ray bina…

2017 The Astrophysical Journal
Gaia 29
A 13CO Detection in a Brightest Cluster Galaxy
DOI: 10.3847/1538-4357/aa8fd0 Bibcode: 2017ApJ...848..101V

Fabian, A. C.; Combes, F.; McDonald, M. +7 more

We present ALMA Cycle 4 observations of CO(1-0), CO(3-2), and 13CO(3-2) line emission in the brightest cluster galaxy (BCG) of RXJ0821+0752. This is one of the first detections of 13CO line emission in a galaxy cluster. Half of the CO(3-2) line emission originates from two clumps of molecular gas that are spatially offset fro…

2017 The Astrophysical Journal
eHST 29
CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
DOI: 10.3847/2041-8213/aa70e9 Bibcode: 2017ApJ...841L..22G

Papovich, Casey; Pérez-González, Pablo G.; Santini, Paola +17 more

We investigate the environmental quenching of galaxies, especially those with stellar masses (M *) < 109.5 M , beyond the local universe. Essentially all local low-mass quenched galaxies (QGs) are believed to live close to massive central galaxies, which is a demonstration of environmental quenching. We use CAN…

2017 The Astrophysical Journal
eHST 29
A Likely Redback Millisecond Pulsar Counterpart of 3FGL J0838.8-2829
DOI: 10.3847/1538-4357/aa7cff Bibcode: 2017ApJ...844..150H

Halpern, J. P.; Strader, J.; Li, M.

We obtained new optical observations of the X-ray source XMMU J083850.38-282756.8, the previously proposed counterpart of the γ-ray source 3FGL J0838.8-2829. Time-series photometry in the r\prime band reveals periodic modulation of ≈ 1 mag that is characteristic of the heating of the photosphere of a low-mass companion star by a compact…

2017 The Astrophysical Journal
XMM-Newton 29
The heterogeneous coma of comet 67P/Churyumov-Gerasimenko as seen by ROSINA: H2O, CO2, and CO from September 2014 to February 2016
DOI: 10.1051/0004-6361/201629900 Bibcode: 2017A&A...600A..77H

Lasue, J.; Wurz, P.; Altwegg, K. +25 more

Context. The ESA Rosetta mission has been investigating the environment of comet 67P/Churyumov-Gerasimenko (67P) since August 2014. Among the experiments on board the spacecraft, the ROSINA experiment (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) includes two mass spectrometers to analyse the composition of neutrals and ions and a CO…

2017 Astronomy and Astrophysics
Rosetta 29
Extremely late photometry of the nearby SN 2011fe
DOI: 10.1093/mnras/stx1923 Bibcode: 2017MNRAS.472.2534K

Spyromilio, J.; Fransson, C.; Jerkstrand, A. +6 more

Type Ia supernovae are widely accepted to be the outcomes of thermonuclear explosions in white dwarf stars. However, many details of these explosions remain uncertain (e.g. the mass, ignition mechanism and flame speed). Theory predicts that at very late times (beyond 1000 d) it might be possible to distinguish between explosion models. Few very ne…

2017 Monthly Notices of the Royal Astronomical Society
eHST 29