Search Publications

Radio Follow-up on All Unassociated Gamma-Ray Sources from the Third Fermi Large Area Telescope Source Catalog
DOI: 10.3847/1538-4357/aa6439 Bibcode: 2017ApJ...838..139S

Edwards, Philip G.; Petrov, Leonid; Schinzel, Frank K. +1 more

The third Fermi Large Area Telescope γ-ray source catalog (3FGL) contains over 1000 objects for which there is no known counterpart at other wavelengths. The physical origin of the γ-ray emission from those objects is unknown. Such objects are commonly referred to as unassociated and mostly do not exhibit significant γ-ray flux variability. We per…

2017 The Astrophysical Journal
Gaia 41
Constraints on the Distance Moduli, Helium, and Metal Abundances, and Ages of Globular Clusters from Their RR Lyrae and Non-variable Horizontal Branch Stars. II. Multiple Stellar Populations in 47 Tuc, M3, and M13
DOI: 10.3847/1538-4357/aa92c9 Bibcode: 2017ApJ...849..159D

VandenBerg, Don A.; Denissenkov, Pavel A.; Kopacki, Grzegorz +1 more

We present a new set of horizontal branch (HB) models computed with the MESA stellar evolution code. The models adopt α-enhanced Asplund et al. metal mixtures and include the gravitational settling of He. They are used in our HB population synthesis tool to generate theoretical distributions of HB stars in order to describe the multiple stellar po…

2017 The Astrophysical Journal
eHST 41
Multiwavelength Study of the Star Formation in the S237 H II Region
DOI: 10.3847/1538-4357/834/1/22 Bibcode: 2017ApJ...834...22D

Dewangan, L. K.; Ojha, D. K.; Zinchenko, I. +2 more

We present a detailed multiwavelength study of observations from X-ray, near-infrared, and centimeter wavelengths to probe the star formation processes in the S237 region. Multiwavelength images trace an almost sphere-like shell morphology of the region, which is filled with the 0.5-2 keV X-ray emission. The region contains two distinct environmen…

2017 The Astrophysical Journal
Herschel 41
The Young L Dwarf 2MASS J11193254-1137466 Is a Planetary-mass Binary
DOI: 10.3847/2041-8213/aa76df Bibcode: 2017ApJ...843L...4B

Magnier, Eugene A.; Dupuy, Trent J.; Liu, Michael C. +1 more

We have discovered that the extremely red, low-gravity L7 dwarf 2MASS J11193254-1137466 is a 0.″14 (3.6 au) binary using Keck laser guide star adaptive optics imaging. 2MASS J11193254-1137466 has previously been identified as a likely member of the TW Hydrae Association (TWA). Using our updated photometric distance and proper motion, a kinematic a…

2017 The Astrophysical Journal
Gaia 41
The AGN-Star Formation Connection: Future Prospects with JWST
DOI: 10.3847/1538-4357/aa911d Bibcode: 2017ApJ...849..111K

Barro, Guillermo; Santini, Paola; Grogin, Norman A. +13 more

The bulk of the stellar growth over cosmic time is dominated by IR-luminous galaxies at cosmic noon (z=1{--}2), many of which harbor a hidden active galactic nucleus (AGN). We use state-of-the-art infrared color diagnostics, combining Spitzer and Herschel observations, to separate dust-obscured AGNs from dusty star-forming galaxies (SFGs) in the C…

2017 The Astrophysical Journal
Herschel 40
Characterizing the Transition from Diffuse Atomic to Dense Molecular Clouds in the Magellanic Clouds with [C II], [C I], and CO
DOI: 10.3847/1538-4357/aa683a Bibcode: 2017ApJ...839..107P

Ott, Jürgen; Hughes, Annie; Wong, Tony +8 more

We present and analyze deep Herschel/HIFI observations of the [C II] 158 µm, [C I] 609 µm, and [C I] 370 µm lines toward 54 lines of sight in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). These observations are used to determine the physical conditions of the line-emitting gas, which we use to study the trans…

2017 The Astrophysical Journal
Herschel 40
New Evidence for a Coronal Mass Ejection-driven High Frequency Type II Burst near the Sun
DOI: 10.3847/1538-4357/aa72e7 Bibcode: 2017ApJ...843...10K

Kumari, Anshu; Ramesh, R.; Kathiravan, C. +1 more

We report observations of the high frequency type II radio burst (≈430-30 MHz) that occurred in the solar corona on 2015 November 4. The drift rate of the burst, estimated close to the start frequency of its fundamental component (≈215 MHz), is unusually high (≈2 MHz s-1). Our analysis shows that the estimated speed of the magnetohydrod…

2017 The Astrophysical Journal
SOHO 40
Turbulent Transport in a Three-dimensional Solar Wind
DOI: 10.3847/1538-4357/aa60bc Bibcode: 2017ApJ...837...75S

Bruno, R.; Zank, G. P.; Shiota, D. +3 more

Turbulence in the solar wind can play essential roles in the heating of coronal and solar wind plasma and the acceleration of the solar wind and energetic particles. Turbulence sources are not well understood and thought to be partly enhanced by interaction with the large-scale inhomogeneity of the solar wind and the interplanetary magnetic field …

2017 The Astrophysical Journal
Ulysses 40
A High Space Density of Luminous Lyman Alpha Emitters at z ∼ 6.5
DOI: 10.3847/1538-4357/837/1/11 Bibcode: 2017ApJ...837...11B

Bagley, Micaela B.; Martin, Crystal L.; Garel, Thibault +16 more

We present the results of a systematic search for Lyα emitters (LAEs) at 6≲ z≲ 7.6 using the HST WFC3 Infrared Spectroscopic Parallel (WISP) Survey. Our total volume over this redshift range is ∼ 8× {10}5 Mpc3, comparable to many of the narrowband surveys despite their larger area coverage. We find two LAEs at z = 6.38 and 6.…

2017 The Astrophysical Journal
eHST 40
Carbon Chain Anions and the Growth of Complex Organic Molecules in Titan’s Ionosphere
DOI: 10.3847/2041-8213/aa7851 Bibcode: 2017ApJ...844L..18D

Lewis, G. R.; Coates, A. J.; Kataria, D. O. +13 more

Cassini discovered a plethora of neutral and ionized molecules in Titan’s ionosphere including, surprisingly, anions and negatively charged molecules extending up to 13,800 u q-1. In this Letter, we forward model the Cassini electron spectrometer response function to this unexpected ionospheric component to achieve an increased mass res…

2017 The Astrophysical Journal
Cassini 40