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Herschel Observations of Gas and Dust in the Unusual 49 Ceti Debris Disk
DOI: 10.1088/0004-637X/771/1/69 Bibcode: 2013ApJ...771...69R

Dent, W. R. F.; Woitke, P.; Kamp, I. +12 more

We present far-IR/sub-mm imaging and spectroscopy of 49 Ceti, an unusual circumstellar disk around a nearby young A1V star. The system is famous for showing the dust properties of a debris disk, but the gas properties of a low-mass protoplanetary disk. The data were acquired with the Herschel Space Observatory PACS and SPIRE instruments, largely a…

2013 The Astrophysical Journal
Herschel 57
Water Vapor in the Protoplanetary Disk of DG Tau
DOI: 10.1088/2041-8205/766/1/L5 Bibcode: 2013ApJ...766L...5P

Pinte, C.; Ménard, F.; Woitke, P. +13 more

Water is key in the evolution of protoplanetary disks and the formation of comets and icy/water planets. While high-excitation water lines originating in the hot inner disk have been detected in several T Tauri stars (TTSs), water vapor from the outer disk, where most water ice reservoirs are stored, was only reported in the nearby TTS TW Hya. We …

2013 The Astrophysical Journal
Herschel 57
Superluminous X-Rays from a Superluminous Supernova
DOI: 10.1088/0004-637X/771/2/136 Bibcode: 2013ApJ...771..136L

Read, A. M.; Wheatley, P. J.; Levan, A. J. +2 more

The discovery of a population of superluminous supernovae (SLSNe), with peak luminosities a factor of ~100 brighter than normal supernovae (SNe; typically SLSNe have MV < -21), has shown an unexpected diversity in core-collapse SN properties. Numerous models have been postulated for the nature of these events, including a strong inte…

2013 The Astrophysical Journal
XMM-Newton 57
Plasma Composition in a Sigmoidal Anemone Active Region
DOI: 10.1088/0004-637X/778/1/69 Bibcode: 2013ApJ...778...69B

van Driel-Gesztelyi, L.; Démoulin, P.; Baker, D. +4 more

Using spectra obtained by the EUV Imaging Spectrometer (EIS) instrument onboard Hinode, we present a detailed spatially resolved abundance map of an active region (AR)-coronal hole (CH) complex that covers an area of 359'' × 485''. The abundance map provides first ionization potential (FIP) bias levels in various coronal structures within the larg…

2013 The Astrophysical Journal
Hinode SOHO 57
Herschel's "Cold Debris Disks": Background Galaxies or Quiescent Rims of Planetary Systems?
DOI: 10.1088/0004-637X/772/1/32 Bibcode: 2013ApJ...772...32K

Krivov, A. V.; Eiroa, C.; Löhne, T. +24 more

Infrared excesses associated with debris disk host stars detected so far peak at wavelengths around ~100 µm or shorter. However, 6 out of 31 excess sources studied in the Herschel Open Time Key Programme, DUNES, have been seen to show significant—and in some cases extended—excess emission at 160 µm, which is larger than the 100 µ…

2013 The Astrophysical Journal
AKARI Herschel eHST 57
Sensitive Search for Radio Variables and Transients in the Extended Chandra Deep Field South
DOI: 10.1088/0004-637X/768/2/165 Bibcode: 2013ApJ...768..165M

Frail, D. A.; Kulkarni, S. R.; Horesh, A. +3 more

We report on an analysis of the Extended Chandra Deep Field South (E-CDFS) region using archival data from the Very Large Array, with the goal of studying radio variability and transients at the sub-milliJansky level. The 49 epochs of E-CDFS observations at 1.4 GHz sample timescales from 1 day to 3 months. We find that only a fraction (1%) of unre…

2013 The Astrophysical Journal
eHST 56
Probing the Extreme Realm of Active Galactic Nucleus Feedback in the Massive Galaxy Cluster, RX J1532.9+3021
DOI: 10.1088/0004-637X/777/2/163 Bibcode: 2013ApJ...777..163H

von der Linden, A.; Fabian, A. C.; Hlavacek-Larrondo, J. +7 more

We present a detailed Chandra, XMM-Newton, Very Large Array (VLA) and Hubble Space Telescope analysis of one of the strongest cool core clusters known, RX J1532.9+3021 (z = 0.3613). Using new, deep 90 ks Chandra observations, we confirm the presence of a western X-ray cavity or bubble, and report on a newly discovered eastern X-ray cavity. The tot…

2013 The Astrophysical Journal
XMM-Newton eHST 56
Phobos as a D-type Captured Asteroid, Spectral Modeling from 0.25 to 4.0 µm
DOI: 10.1088/0004-637X/777/2/127 Bibcode: 2013ApJ...777..127P

Pajola, M.; Barbieri, C.; Bertini, I. +6 more

This paper describes the spectral modeling of the surface of Phobos in the wavelength range between 0.25 and 4.0 µm. We use complementary data to cover this spectral range: the OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System on board the ESA Rosetta spacecraft) reflectance spectrum that Pajola et al. merged with the VSK-KR…

2013 The Astrophysical Journal
Rosetta 56
Active Galactic Nucleus Black Hole Mass Estimates in the Era of Time Domain Astronomy
DOI: 10.1088/0004-637X/779/2/187 Bibcode: 2013ApJ...779..187K

Treu, Tommaso; Malkan, Matthew; Kelly, Brandon C. +2 more

We investigate the dependence of the normalization of the high-frequency part of the X-ray and optical power spectral densities (PSDs) on black hole mass for a sample of 39 active galactic nuclei (AGNs) with black hole masses estimated from reverberation mapping or dynamical modeling. We obtained new Swift observations of PG 1426+015, which has th…

2013 The Astrophysical Journal
XMM-Newton 56
Outflows from Evolved Stars: The Rapidly Changing Fingers of CRL 618
DOI: 10.1088/0004-637X/772/1/20 Bibcode: 2013ApJ...772...20B

Frank, Adam; Corradi, Romano L. M.; Balick, Bruce +4 more

Our ultimate goal is to probe the nature of the collimator of the outflows in the pre-planetary nebula CRL 618. CRL 618 is uniquely suited for this purpose owing to its multiple, bright, and carefully studied finger-shaped outflows east and west of its nucleus. We compare new Hubble Space Telescope images to images in the same filters observed as …

2013 The Astrophysical Journal
eHST 56