Search Publications

Almost gone: SN 2008S and NGC 300 2008OT-1 are fainter than their progenitors
DOI: 10.1093/mnras/stw1059 Bibcode: 2016MNRAS.460.1645A

Kochanek, C. S.; Stanek, K. Z.; Shappee, B. J. +3 more

We present late-time Hubble and Spitzer Space Telescope (SST) imaging of SN 2008S and NGC 300 2008OT-1, the prototypes of a common class of stellar transients whose true nature is debated. Both objects are still fading and are now >15 times fainter than their progenitors in the mid-IR and are undetected in the optical and near-IR. Data from the…

2016 Monthly Notices of the Royal Astronomical Society
eHST 62
Evidence for Intermediate Polars as the Origin of the Galactic Center Hard X-ray Emission
DOI: 10.3847/0004-637X/826/2/160 Bibcode: 2016ApJ...826..160H

Hailey, Charles J.; Mori, Kaya; Zhang, Shuo +14 more

Recently, unresolved hard (20-40 keV) X-ray emission has been discovered within the central 10 pc of the Galaxy, possibly indicating a large population of intermediate polars (IPs). Chandra and XMM-Newton measurements in the surrounding ∼50 pc imply a much lighter population of IPs with < {M}{{WD}}> ≈ 0.5{M}. Here we …

2016 The Astrophysical Journal
INTEGRAL XMM-Newton 62
Dissecting the High-z Interstellar Medium through Intensity Mapping Cross-correlations
DOI: 10.3847/1538-4357/833/2/153 Bibcode: 2016ApJ...833..153S

Lagache, Guilaine; Doré, Olivier; Serra, Paolo

We explore the detection, with upcoming spectroscopic surveys, of three-dimensional power spectra of emission line fluctuations produced in different phases of the interstellar medium (ISM) by forbidden transitions of ionized carbon [C II] (157.7 µm), ionized nitrogen [N II] (121.9 and 205.2 µm), and neutral oxygen [O I] (145.5 µ…

2016 The Astrophysical Journal
ISO 62
The 2016 Feb 19 outburst of comet 67P/CG: an ESA Rosetta multi-instrument study
DOI: 10.1093/mnras/stw2088 Bibcode: 2016MNRAS.462S.220G

Jorda, L.; Lamy, P. L.; Stern, S. A. +93 more

On 2016 Feb 19, nine Rosetta instruments serendipitously observed an outburst of gas and dust from the nucleus of comet 67P/Churyumov-Gerasimenko. Among these instruments were cameras and spectrometers ranging from UV over visible to microwave wavelengths, in situ gas, dust and plasma instruments, and one dust collector. At 09:40 a dust cloud deve…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 62
A Case Against Spinning PAHs as the Source of the Anomalous Microwave Emission
DOI: 10.3847/0004-637X/827/1/45 Bibcode: 2016ApJ...827...45H

Meisner, Aaron M.; Draine, B. T.; Hensley, Brandon S.

We employ an all-sky map of the anomalous microwave emission (AME) produced by component separation of the microwave sky to study correlations between the AME and Galactic dust properties. We find that while the AME is highly correlated with all tracers of dust emission, the best predictor of the AME strength is the dust radiance. Fluctuations in …

2016 The Astrophysical Journal
Planck 62
The dust-scattering component of X-ray extinction: effects on continuum fitting and high-resolution absorption edge structure
DOI: 10.1093/mnras/stw376 Bibcode: 2016MNRAS.458.1345C

García, J.; Wilms, J.; Baganoff, F. +1 more

Small angle scattering by dust grains causes a significant contribution to the total interstellar extinction for any X-ray instrument with sub-arcminute resolution (Chandra, Swift, XMM-Newton). However, the dust-scattering component is not included in the current absorption models: phabs, TBabs, and TBnew. We simulate a large number of Chandra spe…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 62
What Can We Learn about Magnetotail Reconnection from 2D PIC Harris-Sheet Simulations?
DOI: 10.1007/s11214-015-0154-y Bibcode: 2016SSRv..199..651G

Goldman, M. V.; Newman, D. L.; Lapenta, G.

The Magnetosphere Multiscale Mission (MMS) will provide the first opportunity to probe electron-scale physics during magnetic reconnection in Earth's magnetopause and magnetotail. This article will address only tail reconnection—as a non-steady-state process in which the first reconnected field lines advance away from the x-point in flux pile-up f…

2016 Space Science Reviews
Cluster 62
Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates
DOI: 10.1051/0004-6361/201527206 Bibcode: 2016A&A...596A.100P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +188 more

The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources on the sky, including distant objects in the high-redshift Universe traced by their dust emission. A novel method, based on a component-separation procedure using a combi…

2016 Astronomy and Astrophysics
Planck 62
NuSTAR Hard X-Ray Survey of the Galactic Center Region. II. X-Ray Point Sources
DOI: 10.3847/0004-637X/825/2/132 Bibcode: 2016ApJ...825..132H

Hailey, Charles J.; Mori, Kaya; Giommi, Paolo +41 more

We present the first survey results of hard X-ray point sources in the Galactic Center (GC) region by NuSTAR. We have discovered 70 hard (3-79 keV) X-ray point sources in a 0.6 deg{}2 region around Sgr A* with a total exposure of 1.7 Ms, and 7 sources in the Sgr B2 field with 300 ks. We identify clear Chandra counterparts for 58 NuSTAR …

2016 The Astrophysical Journal
XMM-Newton 62
Another piece of the puzzle: The fast H I outflow in Mrk 231
DOI: 10.1051/0004-6361/201628978 Bibcode: 2016A&A...593A..30M

Veilleux, Sylvain; Morganti, Raffaella; Oosterloo, Tom +2 more

We present the detection, performed with the Westerbork Synthesis Radio Telescope (WSRT) and the Karl Jansky Very Large Array (VLA), of a fast H I 21 cm outflow in the ultra-luminous infrared galaxy Mrk 231. The outflow is observed as shallow H I absorption blueshifted ~1300 km s-1 with respect to the systemic velocity and located again…

2016 Astronomy and Astrophysics
eHST 62