Search Publications

Simultaneous Multiwavelength Observations of V404 Cygni during its 2015 June Outburst Decay Strengthen the Case for an Extremely Energetic Jet-base
DOI: 10.3847/1538-4357/aa98a0 Bibcode: 2017ApJ...851..148M

Maccarone, Thomas J.; Grinberg, Victoria; Reynolds, Mark T. +4 more

We present results of multiband optical photometry of the black hole X-ray binary system V404 Cyg obtained using Wheaton College Observatory’s 0.3 m telescope, along with strictly simultaneous INTEGRAL and Swift observations during 2015 June 25.15-26.33 UT, and 2015 June 27.10-27.34 UT. These observations were made during the 2015 June outburst of…

2017 The Astrophysical Journal
INTEGRAL 14
Reverberation Mapping of PG 0934+013 with the Southern African Large Telescope
DOI: 10.3847/1538-4357/aa88a3 Bibcode: 2017ApJ...847..125P

Barth, Aaron J.; Im, Myungshin; Jeon, Yiseul +10 more

We present the variability and time-lag measurements of PG 0934+013 based on a photometric and spectroscopic monitoring campaign over a two year period. We obtained 46 epochs of data from the spectroscopic campaign, which was carried out using the Southern African Large Telescope with ∼1 week cadence over two sets of four month-long observing peri…

2017 The Astrophysical Journal
eHST 14
A Spectroscopic Orbit for the Late-type Be Star β CMi
DOI: 10.3847/1538-4357/836/1/112 Bibcode: 2017ApJ...836..112D

Wang, Luqian; Klement, Robert; Richardson, Noel D. +12 more

The late-type Be star β CMi is remarkably stable compared to other Be stars that have been studied. This has led to a realistic model of the outflowing Be disk by Klement et al. These results showed that the disk is likely truncated at a finite radius from the star, which Klement et al. suggest is evidence for an unseen binary companion in orbit. …

2017 The Astrophysical Journal
IUE 14
Evolution of Dust-obscured Star Formation and Gas to z = 2.2 from HiZELS
DOI: 10.3847/1538-4357/aa61a6 Bibcode: 2017ApJ...838..119T

Thomson, A. P.; Smail, Ian; Ibar, E. +6 more

We investigate the far-infrared (far-IR) properties of galaxies selected via deep, narrow-band imaging of the Hα emission line in four redshift slices from z=0.40{--}2.23 over ∼1 deg2 as part of the High-redshift Emission Line Survey (HiZELS). We use a stacking approach in the Herschel PACS/SPIRE far-IR bands, along with 850 µ {{m…

2017 The Astrophysical Journal
Herschel 14
High-resolution Observations of a White-light Flare with NST
DOI: 10.3847/1538-4357/aa633f Bibcode: 2017ApJ...838...32Y

Cho, K. -S.; Xu, Y.; Yurchyshyn, V. +4 more

Using high-resolution data from the New Solar Telescope, we studied fine spatial and temporal details of an M1.3 white-light (WL) flare, which was one of three homologous solar flares (C6.8, M1.3, and M2.3) observed in close proximity to the west solar limb on 2014 October 29 in NOAA active region 12192. We report that the TiO WL flare consists of…

2017 The Astrophysical Journal
Hinode 14
Development of a Full Ice-cream Cone Model for Halo Coronal Mass Ejections
DOI: 10.3847/1538-4357/aa697c Bibcode: 2017ApJ...839...82N

Moon, Y. -J.; Lee, Harim; Na, Hyeonock

It is essential to determine three-dimensional parameters (e.g., radial speed, angular width, and source location) of coronal mass ejections (CMEs) for the space weather forecast. In this study, we investigate which cone type represents a halo CME morphology using 29 CMEs (12 Solar and Heliospheric Observatory (SOHO)/Large Angle and Spectrometric …

2017 The Astrophysical Journal
SOHO 14
On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary
DOI: 10.3847/1538-4357/aa7e79 Bibcode: 2017ApJ...845...39O

Hamann, W. -R.; Oskinova, L. M.; Ignace, R. +5 more

The blue hypergiant Cyg OB2 12 (B3Ia+) is a representative member of the class of very massive stars in a poorly understood evolutionary stage. We obtained its high-resolution X-ray spectrum using the Chandra observatory. PoWR model atmospheres were calculated to provide realistic wind opacities and to establish the wind density structu…

2017 The Astrophysical Journal
ISO 14
The First Detection of a Pulsar with ALMA
DOI: 10.3847/2041-8213/aa9c3e Bibcode: 2017ApJ...851L..10M

de Luca, A.; Possenti, A.; Burgay, M. +8 more

Although there is a general consensus on the fact that pulsars’ radio emission is coherent in nature, whereas the emission from the optical to high-energy γ-rays is due to incoherent processes, it has not been established yet at which wavelengths the transition occurs, which is key information for all emission models of pulsar magnetospheres. Of c…

2017 The Astrophysical Journal
eHST 14
A Tale of Two Impostors: SN2002kg and SN1954J in NGC 2403
DOI: 10.3847/1538-4357/aa8a71 Bibcode: 2017ApJ...848...86H

Van Dyk, Schuyler D.; Humphreys, Roberta M.; Davidson, Kris +1 more

We describe new results on two supernova impostors in NGC 2403, SN 1954J(V12) and SN 2002kg(V37). For the famous object SN 1954J, we combine four critical observations: its current SED, its Hα emission line profile, the Ca II triplet in absorption in its red spectrum, and the brightness compared to its pre-event state. Together, these strongly sug…

2017 The Astrophysical Journal
eHST 14
ALMA Observations of the Gravitational Lens SDP.9
DOI: 10.3847/2041-8213/aa7d4a Bibcode: 2017ApJ...843L..35W

Tamura, Yoichi; Oguri, Masamune; Matsushita, Satoki +3 more

We present long-baseline ALMA observations of the strong gravitational lens H-ATLAS J090740.0-004200 (SDP.9), which consists of an elliptical galaxy at {z}{{L}}=0.6129 lensing a background submillimeter galaxy into two extended arcs. The data include Band 6 continuum observations, as well as CO J = 6-5 molecular line observations, from …

2017 The Astrophysical Journal
eHST 14