Search Publications

A Decade of MWC 758 Disk Images: Where Are the Spiral-arm-driving Planets?
DOI: 10.3847/2041-8213/aab7f5 Bibcode: 2018ApJ...857L...9R

Debes, John H.; Schneider, Glenn; Esposito, Thomas M. +10 more

Large-scale spiral arms have been revealed in scattered light images of a few protoplanetary disks. Theoretical models suggest that such arms may be driven by and corotate with giant planets, which has called for remarkable observational efforts to look for them. By examining the rotation of the spiral arms for the MWC 758 system over a 10 year ti…

2018 The Astrophysical Journal
eHST 27
Reconnection in the Post-impulsive Phase of Solar Flares
DOI: 10.3847/1538-4357/aabad4 Bibcode: 2018ApJ...858...70F

Reeves, Katharine K.; Forbes, Terry G.; Seaton, Daniel B.

Using a recently developed analytical procedure, we determine the rate of magnetic reconnection in the “standard” model of eruptive solar flares. During the late phase, the neutral line is located near the lower tip of the reconnection current sheet, and the upper region of the current sheet is bifurcated into a pair of Petschek-type shocks. Despi…

2018 The Astrophysical Journal
Hinode 27
The Optical/Near-infrared Extinction Law in Highly Reddened Regions
DOI: 10.3847/1538-4357/aaabbb Bibcode: 2018ApJ...855...13H

Hosek, Matthew W., Jr.; Lu, Jessica R.; Clarkson, William I. +6 more

A precise extinction law is a critical input when interpreting observations of highly reddened sources such as young star clusters and the Galactic Center (GC). We use Hubble Space Telescope observations of a region of moderate extinction and a region of high extinction to measure the optical and near-infrared extinction law (0.8-2.2 µm). Th…

2018 The Astrophysical Journal
eHST 27
Outflowing OH+ in Markarian 231: The Ionization Rate of the Molecular Gas
DOI: 10.3847/1538-4357/aab6b8 Bibcode: 2018ApJ...857...66G

Sturm, E.; Veilleux, S.; Ashby, M. L. N. +6 more

The oxygen-bearing molecular ions OH+, H2O+, and H3O+ are key species that probe the ionization rate of (partially) molecular gas that is ionized by X-rays and cosmic-rays permeating the interstellar medium. We report Herschel far-infrared and submillimeter spectroscopic observations of OH

2018 The Astrophysical Journal
Herschel 27
Chemical Abundances in the Leading Arm of the Magellanic Stream
DOI: 10.3847/1538-4357/aaa9bb Bibcode: 2018ApJ...854..142F

Richter, Philipp; Lockman, Felix J.; Fox, Andrew J. +8 more

The Leading Arm (LA) of the Magellanic Stream is a vast debris field of H I clouds connecting the Milky Way and the Magellanic Clouds. It represents an example of active gas accretion onto the Galaxy. Previously, only one chemical abundance measurement had been made in the LA. Here we present chemical abundance measurements using Hubble Space Tele…

2018 The Astrophysical Journal
eHST 27
A Dust-scattering Halo of 4U 1630-47 Observed with Chandra and Swift: New Constraints on the Source Distance
DOI: 10.3847/1538-4357/aabcd3 Bibcode: 2018ApJ...859...88K

Maccarone, T. J.; Tomsick, J. A.; Kalemci, E.

We have observed the Galactic black hole transient 4U 1630-47 during the decay of its 2016 outburst with Chandra and Swift to investigate the properties of the dust-scattering halo created by the source. The scattering halo shows a structure that includes a bright ring between 80″ and 240″ surrounding the source, and a continuous distribution beyo…

2018 The Astrophysical Journal
Planck 27
Gravitationally Unstable Condensations Revealed by ALMA in the TUKH122 Prestellar Core in the Orion A Cloud
DOI: 10.3847/1538-4357/aab3d0 Bibcode: 2018ApJ...856..147O

Sanhueza, Patricio; Choi, Minho; Tatematsu, Ken'ichi +5 more

We have investigated the TUKH122 prestellar core in the Orion A cloud using ALMA 3 mm dust continuum, N2H+ (J = 1-0), and CH3OH ({J}K={2}K-{1}K) molecular-line observations. Previous studies showed that TUKH122 is likely on the verge of star formation because the turbulence is almos…

2018 The Astrophysical Journal
Herschel 27
CO in Protostars (COPS): Herschel-SPIRE Spectroscopy of Embedded Protostars
DOI: 10.3847/1538-4357/aac2c6 Bibcode: 2018ApJ...860..174Y

Larson, Rebecca L.; Lee, Jeong-Eun; Bouwman, Jeroen +13 more

We present full spectral scans from 200 to 670 µm of 26 Class 0+I protostellar sources obtained with Herschel-SPIRE as part of the “COPS-SPIRE” Open Time program, complementary to the DIGIT and WISH Key Programs. Based on our nearly continuous, line-free spectra from 200 to 670 µm, the calculated bolometric luminosities (L bol

2018 The Astrophysical Journal
Herschel 27
A Stealth CME Bracketed between Slow and Fast Wind Producing Unexpected Geoeffectiveness
DOI: 10.3847/1538-4357/aac381 Bibcode: 2018ApJ...860...78H

Wang, Rui; Liu, Ying D.; Hu, Huidong +2 more

We investigate how a weak coronal mass ejection (CME) launched on 2016 October 8 without obvious signatures in the low corona produced a relatively intense geomagnetic storm. Remote sensing observations from SDO, STEREO, and SOHO and in situ measurements from Wind are employed to track the CME from the Sun to the Earth. Using a graduated cylindric…

2018 The Astrophysical Journal
SOHO 27
Variable Nature of Magnetically Driven Ultra-fast Outflows
DOI: 10.3847/2041-8213/aadd10 Bibcode: 2018ApJ...864L..27F

Behar, Ehud; Tombesi, Francesco; Shrader, Chris +3 more

Among a number of active galactic nuclei that drive ionized outflows in X-rays, a low-redshift (z = 0.184) quasar, PDS 456, is long known to exhibit one of the exemplary ultra-fast outflows (UFOs). However, the physical process of acceleration mechanisms is yet to be definitively constrained. In this work, we model the variations of the Fe K UFO p…

2018 The Astrophysical Journal
XMM-Newton 27