Search Publications

ALMA 26 Arcmin2 Survey of GOODS-S at One Millimeter (ASAGAO): Average Morphology of High-z Dusty Star-forming Galaxies in an Exponential Disk (n ≃ 1)
DOI: 10.3847/1538-4357/aac6c4 Bibcode: 2018ApJ...861....7F

Ouchi, Masami; Ivison, R. J.; Dunlop, J. S. +23 more

We present morphological properties of dusty star-forming galaxies at z = 1-3 determined with the high-resolution (FWHM ∼ 0.″19) Atacama Large Milllimeter/submillimeter Array (ALMA) 1 mm map of our ASAGAO survey covering a 26 arcmin2 area in GOODS-S. In conjunction with the ALMA archival data, our sample consists of 45 ALMA sources with…

2018 The Astrophysical Journal
Gaia Herschel eHST 51
Characterizing TW Hydra
DOI: 10.3847/1538-4357/aaa1e4 Bibcode: 2018ApJ...853..120S

Lee, Jae-Joon; Kim, Hwihyun; Jaffe, Daniel T. +5 more

At 60 pc, TW Hydra (TW Hya) is the closest example of a star with a gas-rich protoplanetary disk, though TW Hya may be relatively old (3-15 Myr). As such, TW Hya is especially appealing for testing our understanding of the interplay between stellar and disk evolution. We present a high-resolution near-infrared spectrum of TW Hya obtained with the …

2018 The Astrophysical Journal
Gaia 51
Periastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year Period
DOI: 10.3847/2041-8213/aae70e Bibcode: 2018ApJ...867L..19A

Maraschi, L.; Covino, S.; Antonelli, L. A. +211 more

We report on observations of the pulsar/Be star binary system PSR J2032+4127/MT91 213 in the energy range between 100 {GeV} and 20 {TeV} with the Very Energetic Radiation Imaging Telescope Array and Major Atmospheric Gamma Imaging Cherenkov telescope arrays. The binary orbit has a period of approximately 50 years, with the most recent periastron o…

2018 The Astrophysical Journal
Gaia 51
Element Abundance Ratios in the Quiet Sun Transition Region
DOI: 10.3847/1538-4357/aaab48 Bibcode: 2018ApJ...855...15Y

Young, P. R.

Element abundance ratios of magnesium to neon (Mg/Ne) and neon to oxygen (Ne/O) in the transition region of the quiet Sun have been derived by re-assessing previously published data from the Coronal Diagnostic Spectrometer on board the Solar and Heliospheric Observatory in the light of new atomic data. The quiet Sun Mg/Ne ratio is important for as…

2018 The Astrophysical Journal
SOHO 51
Interrogating Seyferts with NebulaBayes: Spatially Probing the Narrow-line Region Radiation Fields and Chemical Abundances
DOI: 10.3847/1538-4357/aab3db Bibcode: 2018ApJ...856...89T

Kewley, Lisa J.; Blanc, Guillermo A.; Hopkins, Andrew M. +4 more

NebulaBayes is a new Bayesian code that implements a general method of comparing observed emission-line fluxes to photoionization model grids. The code enables us to extract robust, spatially resolved measurements of abundances in the extended narrow-line regions (ENLRs) produced by Active Galactic Nuclei (AGN). We observe near-constant ionization…

2018 The Astrophysical Journal
eHST 51
Broad Non-Gaussian Fe XXIV Line Profiles in the Impulsive Phase of the 2017 September 10 X8.3-class Flare Observed by Hinode/EIS
DOI: 10.3847/1538-4357/aad62d Bibcode: 2018ApJ...864...63P

Reeves, Katharine K.; Polito, Vanessa; Chen, Bin +4 more

We analyze the spectra of high-temperature Fe XXIV lines observed by the Hinode/Extreme-Ultraviolet Imaging Spectrometer (EIS) during the impulsive phase of the X8.3-class flare on 2017 September 10. The line profiles are broad, show pronounced wings, and clearly depart from a single-Gaussian shape. The lines can be well fitted with κ distribution…

2018 The Astrophysical Journal
Hinode 51
The Orbit of the Companion to HD 100453A: Binary-driven Spiral Arms in a Protoplanetary Disk
DOI: 10.3847/1538-4357/aaa767 Bibcode: 2018ApJ...854..130W

Dong, Ruobing; Wagner, Kevin; Apai, Dániel +9 more

HD 100453AB is a 10 ± 2 Myr old binary whose protoplanetary disk was recently revealed to host a global two-armed spiral structure. Given the relatively small projected separation of the binary (1.″05, or ∼108 au), gravitational perturbations by the binary seemed to be a likely driving force behind the formation of the spiral arms. However, the or…

2018 The Astrophysical Journal
Gaia 50
Breaking the Habit: The Peculiar 2016 Eruption of the Unique Recurrent Nova M31N 2008-12a
DOI: 10.3847/1538-4357/aab6a6 Bibcode: 2018ApJ...857...68H

Sabo, R.; Ness, J. -U.; Henze, M. +70 more

Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an extreme object, with a massive white dwarf and a high accretion rate, which is the most promising candidate for the single-degenerate progenitor of a Type Ia supernova known to date. The pr…

2018 The Astrophysical Journal
XMM-Newton eHST 50
Phlegethon, a Nearby 75°-long Retrograde Stellar Stream
DOI: 10.3847/1538-4357/aadba3 Bibcode: 2018ApJ...865...85I

Malhan, Khyati; Ibata, Rodrigo A.; Martin, Nicolas F. +1 more

We report the discovery of a 75°-long stellar stream in the Gaia DR2 catalog, found using the new STREAMFINDER algorithm. The structure is probably the remnant of a now fully disrupted globular cluster, which lies ≈3.8 kpc away from the Sun in the direction of the Galactic bulge and possesses highly retrograde motion. We find that the system orbit…

2018 The Astrophysical Journal
Gaia 50
New and Known Moving Groups and Clusters Identified in a Gaia Comoving Catalog
DOI: 10.3847/1538-4357/aac76e Bibcode: 2018ApJ...863...91F

Faherty, Jacqueline K.; Gagné, Jonathan; Bochanski, John J. +5 more

We present a reorganization of the Oh et al. wide, comoving catalog of 4555 groups of stars (10,606 individual objects) identified in the Tycho Gaia Astrometric Survey (TGAS) into new and known coevolving groups of stars in the Milky Way. We use the BANYAN Σ kinematic analysis tool to identify 1015 individual stars in the Oh et al. catalog that yi…

2018 The Astrophysical Journal
Gaia Hipparcos 50