Search Publications

Chromospheric Condensation and Quasi-periodic Pulsations in a Circular-ribbon Flare
DOI: 10.3847/0004-637X/832/1/65 Bibcode: 2016ApJ...832...65Z

Li, D.; Zhang, Q. M.; Ning, Z. J.

In this paper, we report our multiwavelength observations of the C3.1 circular-ribbon flare SOL2015-10-16T10:20 in active region (AR) 12434. The flare consisted of a circular flare ribbon (CFR), an inner flare ribbon (IFR) inside it, and a pair of short parallel flare ribbons (PFRs). The PFRs located to the north of the IFR were most striking in t…

2016 The Astrophysical Journal
Hinode IRIS 57
Infrared Spectral Energy Distribution Decomposition of WISE-selected, Hyperluminous Hot Dust-obscured Galaxies
DOI: 10.3847/0004-637X/823/2/107 Bibcode: 2016ApJ...823..107F

Nikutta, Robert; Knudsen, Kirsten K.; Drouart, Guillaume +2 more

We utilize a Bayesian approach to fit the observed mid-IR-to-submillimeter/millimeter spectral energy distributions (SEDs) of 22 WISE-selected and submillimeter-detected, hyperluminous hot dust-obscured galaxies (Hot DOGs), with spectroscopic redshift ranging from 1.7 to 4.6. We compare the Bayesian evidence of a torus plusgraybody (Torus+GB) mode…

2016 The Astrophysical Journal
Herschel 56
On the Metallicity and Origin of the Smith High-velocity Cloud
DOI: 10.3847/2041-8205/816/1/L11 Bibcode: 2016ApJ...816L..11F

Sembach, Kenneth R.; Lockman, Felix J.; Rahman, Mubdi +7 more

The Smith Cloud (SC) is a gaseous high-velocity cloud (HVC) in an advanced state of accretion, only 2.9 kpc below the Galactic plane and due to impact the disk in ≈27 Myr. It is unique among HVCs in having a known distance (12.4 ± 1.3 kpc) and a well-constrained 3D velocity (296 km s-1), but its origin has long remained a mystery. Here …

2016 The Astrophysical Journal
eHST 56
First Gaia Local Group Dynamics: Magellanic Clouds Proper Motion and Rotation
DOI: 10.3847/2041-8205/832/2/L23 Bibcode: 2016ApJ...832L..23V

van der Marel, Roeland P.; Sahlmann, Johannes

We use the Gaia data release 1 (DR1) to study the proper motion (PM) fields of the Large and Small Magellanic Clouds (LMC, SMC). This uses the Tycho-Gaia Astrometric Solution (TGAS) PMs for 29 Hipparcos stars in the LMC and 8 in the SMC. The LMC PM in the West and North directions is inferred to be ({µ }W,{µ }N) =…

2016 The Astrophysical Journal
Gaia eHST 56
Radio Disappearance of the Magnetar XTE J1810-197 and Continued X-ray Timing
DOI: 10.3847/0004-637X/820/2/110 Bibcode: 2016ApJ...820..110C

Camilo, F.; Ransom, S. M.; Johnston, S. +6 more

We report on timing, flux density, and polarimetric observations of the transient magnetar and 5.54 s radio pulsar XTE J1810-197 using the Green Bank, Nançay, and Parkes radio telescopes beginning in early 2006, until its sudden disappearance as a radio source in late 2008. Repeated observations through 2016 have not detected radio pulsations agai…

2016 The Astrophysical Journal
XMM-Newton 56
Determining Ages of APOGEE Giants with Known Distances
DOI: 10.3847/0004-637X/817/1/40 Bibcode: 2016ApJ...817...40F

Bovy, Jo; Majewski, Steven R.; Feuillet, Diane K. +4 more

We present a sample of 705 local giant stars observed using the New Mexico State University 1 m telescope with the Sloan Digital Sky Survey-III/Apache Point Observatory Galactic Evolution Experiment (APOGEE) spectrograph, for which we estimate stellar ages and the local star formation history (SFH). The high-resolution (R ∼ 22,500), near infrared …

2016 The Astrophysical Journal
Hipparcos 56
SN Refsdal: Classification as a Luminous and Blue SN 1987A-like Type II Supernova
DOI: 10.3847/0004-637X/831/2/205 Bibcode: 2016ApJ...831..205K

Zitrin, A.; Filippenko, A. V.; Foley, R. J. +20 more

We have acquired Hubble Space Telescope (HST) and Very Large Telescope near-infrared spectra and images of supernova (SN) Refsdal after its discovery as an Einstein cross in fall 2014. The HST light curve of SN Refsdal has a shape consistent with the distinctive, slowly rising light curves of SN 1987A-like SNe, and we find strong evidence for a br…

2016 The Astrophysical Journal
eHST 55
Origin of Molecular Oxygen in Comet 67P/Churyumov-Gerasimenko
DOI: 10.3847/2041-8205/823/2/L41 Bibcode: 2016ApJ...823L..41M

Wurz, P.; Altwegg, K.; Bieler, A. +13 more

Molecular oxygen has been detected in the coma of comet 67P/Churyumov-Gerasimenko with abundances in the 1%-10% range by the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis-Double Focusing Mass Spectrometer instrument on board the Rosetta spacecraft. Here we find that the radiolysis of icy grains in low-density environments such as the p…

2016 The Astrophysical Journal
Rosetta 55
A Distant Echo of Milky Way Central Activity Closes the Galaxy’s Baryon Census
DOI: 10.3847/2041-8205/828/1/L12 Bibcode: 2016ApJ...828L..12N

Elvis, M.; Nicastro, F.; Krongold, Y. +2 more

We report on the presence of large amounts of million-degree gas in the Milky Way’s interstellar and circum-galactic medium. This gas (1) permeates both the Galactic plane and the halo, (2) extends to distances larger than 60-200 kpc from the center, and (3) its mass is sufficient to close the Galaxy’s baryon census. Moreover, we show that a vast,…

2016 The Astrophysical Journal
XMM-Newton 55
The Wind Nebula around Magnetar Swift J1834.9-0846
DOI: 10.3847/0004-637X/824/2/138 Bibcode: 2016ApJ...824..138Y

Lin, L.; Kouveliotou, C.; Baring, M. G. +12 more

We report on the analysis of two deep XMM-Newton observations of the magnetar Swift J1834.9-0846 and its surrounding extended emission taken in 2014 March and October, 2.5 and 3.1 yr after the source went into outburst. The magnetar is only weakly detected in the first observation, with an absorption-corrected flux {F}0.5-10{keV}≈ 4× {1…

2016 The Astrophysical Journal
XMM-Newton 54