Search Publications

Spectroscopic Confirmation of the Dwarf Spheroidal Galaxy d0994+71 as a Member of the M81 Group of Galaxies
DOI: 10.3847/2041-8205/830/1/L21 Bibcode: 2016ApJ...830L..21T

Simon, Joshua D.; Chiboucas, Kristin; Guhathakurta, Puragra +3 more

We use Keck/DEIMOS spectroscopy to measure the first velocity and metallicity of a dwarf spheroidal (dSph) galaxy beyond the Local Group using resolved stars. Our target, d0944+71, is a faint dSph found in the halo of the massive spiral galaxy M81 by Chiboucas et al. We coadd the spectra of 27 individual stars and measure a heliocentric radial vel…

2016 The Astrophysical Journal
eHST 10
Spectroscopic Diagnostics of Solar Magnetic Flux Ropes Using Iron Forbidden Line
DOI: 10.3847/2041-8205/823/1/L4 Bibcode: 2016ApJ...823L...4C

Cheng, X.; Ding, M. D.

In this Letter, we present Interface Region Imaging Spectrograph Fe xxi 1354.08 Å forbidden line emission of two magnetic flux ropes (MFRs) that caused two fast coronal mass ejections with velocities of ≥1000 km s-1 and strong flares (X1.6 and M6.5) on 2014 September 10 and 2015 June 22, respectively. The extreme-ultraviolet images at t…

2016 The Astrophysical Journal
IRIS 10
New Constraints on the Molecular Gas in the Prototypical HyLIRGs BRI1202-0725 and BRI1335-0417
DOI: 10.3847/0004-637X/830/2/63 Bibcode: 2016ApJ...830...63J

Momjian, E.; Walter, F.; Riechers, D. A. +6 more

We present Karl G Jansky Very Large Array observations of CO(J=2\to 1) line emission and rest-frame 250 GHz continuum emission of the Hyper-Luminous IR Galaxies (HyLIRGs) BRI 1202-0725 (z = 4.69) and BRI 1335-0417 (z = 4.41), with an angular resolution as high as 0.″15. Our low-order CO observations delineate the cool molecular gas, the fuel for s…

2016 The Astrophysical Journal
eHST 10
Major-Merger Galaxy Pairs at Z = 0: Dust Properties and Companion Morphology
DOI: 10.3847/0004-637X/829/2/78 Bibcode: 2016ApJ...829...78D

Domingue, Donovan L.; Cao, Chen; Xu, C. Kevin +4 more

We present an analysis of dust properties of a sample of close major-merger galaxy pairs selected by K s magnitude and redshift. The pairs represent the two populations of spiral-spiral (S+S) and mixed morphology spiral-elliptical (S+E). The Code Investigating GALaxy Emission software is used to fit dust models to the Two Micron All S…

2016 The Astrophysical Journal
Herschel 10
The Optical Variability of SDSS Quasars from Multi-epoch Spectroscopy. III. A Sudden UV Cutoff in Quasar SDSS J2317+0005
DOI: 10.3847/0004-637X/826/2/186 Bibcode: 2016ApJ...826..186G

Prochaska, J. Xavier; Ma, Jingzhe; Malkan, Matthew A. +6 more

We have collected near-infrared to X-ray data of 20 multi-epoch heavily reddened SDSS quasars to investigate the physical mechanism of reddening. Of these, J2317+0005 is found to be a UV cutoff quasar. Its continuum, which usually appears normal, decreases by a factor 3.5 at 3000 Å, compared to its more typical bright state during an interval of 2…

2016 The Astrophysical Journal
XMM-Newton 10
HST STIS Observations of the Mixing Layer in the Cat’s Eye Nebula
DOI: 10.3847/2041-8205/822/1/L19 Bibcode: 2016ApJ...822L..19F

Toalá, Jesús A.; Guerrero, Martín A.; Chu, You-Hua +2 more

Planetary nebulae (PNe) are expected to have a ∼105 K interface layer between the ≥slant 106 K inner hot bubble and the ∼104 K optical nebular shell. The PN structure and evolution, and the X-ray emission, depend critically on the efficiency of the mixing of material at this interface layer. However, neither its lo…

2016 The Astrophysical Journal
eHST 10
Multiple Outflows in the Giant Eruption of a Massive Star
DOI: 10.3847/0004-637X/826/2/191 Bibcode: 2016ApJ...826..191H

Humphreys, Roberta M.; Jones, Terry J.; Gordon, Michael S. +1 more

The supernova impostor PSN J09132750+7627410 in NGC 2748 reached a maximum luminosity of ≈-14 mag. It was quickly realized that it was not a true supernova, but another example of a nonterminal giant eruption. PSN J09132750+7627410 is distinguished by multiple P Cygni absorption minima in the Balmer emission lines that correspond to outflow veloci…

2016 The Astrophysical Journal
eHST 10
Investigating the Circumstellar Disk of the Be Shell Star 48 Librae
DOI: 10.3847/0004-637X/826/1/81 Bibcode: 2016ApJ...826...81S

Okazaki, A. T.; Carciofi, A. C.; Bednarski, D. +6 more

A global disk oscillation implemented in the viscous decretion disk (VDD) model has been used to reproduce most of the observed properties of the well known Be star ζ Tau. 48 Librae shares several similarities with ζ Tau—they are both early-type Be stars, display shell characteristics in their spectra, and exhibit cyclic V/R variations—but has som…

2016 The Astrophysical Journal
AKARI IUE 10
Challenging Some Contemporary Views of Coronal Mass Ejections. I. The Case for Blast Waves
DOI: 10.3847/0004-637X/824/2/92 Bibcode: 2016ApJ...824...92H

Pizzo, V. J.; Howard, T. A.

Since the closure of the “solar flare myth” debate in the mid-1990s, a specific narrative of the nature of coronal mass ejections (CMEs) has been widely accepted by the solar physics community. This narrative describes structured magnetic flux ropes at the CME core that drive the surrounding field plasma away from the Sun. This narrative replaced …

2016 The Astrophysical Journal
SOHO 10
The [Ne III] Jet of DG Tau and its Ionization Scenarios
DOI: 10.3847/0004-637X/832/2/153 Bibcode: 2016ApJ...832..153L

Herczeg, Gregory J.; Liu, Chun-Fan; Shang, Hsien +1 more

Forbidden neon emission from jets of low-mass young stars can be used to probe the underlying high-energy processes in these systems. We analyze spectra of the jet of DG Tau obtained with the Very Large Telescope/X-Shooter spectrograph in 2010. [Ne III] λ 3869 is clearly detected in the innermost 3″ microjet and the outer knot located at ∼ 6\build…

2016 The Astrophysical Journal
eHST 10