Search Publications

Measuring the Magnetic Field of Young Stars Using iSHELL Observations: BP Tau and V347 Aur
DOI: 10.3847/1538-4357/ab35d4 Bibcode: 2019ApJ...882...75F

Flores, C.; Boogert, A.; Connelley, M. S. +1 more

While it has been suggested that there is a connection between the magnetic properties and the internal structure of young stars, there have not been enough magnetic measurements to firmly establish such a correlation at the earliest ages. Here, we contribute to this endeavor by presenting stellar parameters and magnetic field strength measurement…

2019 The Astrophysical Journal
Gaia 22
Broadband Spectral Energy Distributions of SDSS-selected Quasars and of Their Host Galaxies: Intense Activity at the Onset of AGN Feedback
DOI: 10.3847/1538-4357/aaf86b Bibcode: 2019ApJ...871..136B

Lapi, Andrea; Gilli, Roberto; Baccigalupi, Carlo +3 more

We present the mean spectral energy distribution (SED) of a sample of optically selected quasars (QSOs) at redshifts of 1 ≤ z ≤ 5. To derive it, we exploit photometric information from the Sloan Digital Sky Survey, UKIRT Infrared Deep Sky Survey, and Wide-field Infrared Survey Explorer surveys in combination with a stacking analysis of Herschel, A…

2019 The Astrophysical Journal
AKARI Herschel 21
Star Formation Histories of the LEGUS Spiral Galaxies. I. The Flocculent Spiral NGC 7793
DOI: 10.3847/1538-4357/ab1de1 Bibcode: 2019ApJ...878....1S

Cignoni, M.; Tosi, M.; Sabbi, E. +13 more

We present a detailed study of the flocculent spiral galaxy NGC 7793, part of the Sculptor group. By analyzing the resolved stellar populations of the galaxy, located at a distance of ∼3.7 Mpc, we infer for the first time its radial star formation history (SFH) from Hubble Space Telescope photometry, thanks to both archival and new data from the L…

2019 The Astrophysical Journal
eHST 21
A Two-sided Loop X-Ray Solar Coronal Jet Driven by a Minifilament Eruption
DOI: 10.3847/1538-4357/aaf1d3 Bibcode: 2019ApJ...871..220S

Harra, Louise K.; Moore, Ronald L.; Sterling, Alphonse C. +1 more

Most of the commonly discussed solar coronal jets are the type that consist of a single spire extending approximately vertically from near the solar surface into the corona. Recent research supports that eruption of a miniature filament (minifilament) drives many such single-spire jets and concurrently generates a miniflare at the eruption site. A…

2019 The Astrophysical Journal
Hinode 21
Joint X-Ray, EUV, and UV Observations of a Small Microflare
DOI: 10.3847/1538-4357/ab2dfa Bibcode: 2019ApJ...881..109H

Krucker, Säm; White, Stephen M.; Grefenstette, Brian W. +5 more

We present the first joint observation of a small microflare in X-rays with the Nuclear Spectroscopic Telescope ARray (NuSTAR), in UV with the Interface Region Imaging Spectrograph (IRIS), and in EUV with the Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA). These combined observations allow us to study the hot coronal and cooler …

2019 The Astrophysical Journal
IRIS 21
Kinematics of the O VI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
DOI: 10.3847/1538-4357/ab48eb Bibcode: 2019ApJ...886...66N

Charlton, Jane C.; Kacprzak, Glenn G.; Churchill, Christopher W. +4 more

We probe the high-ionization circumgalactic medium by examining absorber kinematics, absorber-galaxy kinematics, and average absorption profiles of 31 O VI absorbers from the “Multiphase Galaxy Halos” Survey as a function of halo mass, redshift, inclination, and azimuthal angle. The galaxies are isolated at 0.12 < z gal < 0.66 and…

2019 The Astrophysical Journal
eHST 21
Changes in Solar Rotation over Two Solar Cycles
DOI: 10.3847/1538-4357/ab3b57 Bibcode: 2019ApJ...883...93B

Basu, Sarbani; Antia, H. M.

We use helioseismic data from ground- and space-based instruments to analyze how solar rotation has changed since the beginning of solar Cycle 23 with emphasis on studying the differences between Cycles 23 and 24. We find that the nature of solar rotation is indeed different for the two cycles. While the changes in the latitudinally independent co…

2019 The Astrophysical Journal
SOHO 21
Noncircular Motions in the Outer Perseus Spiral Arm
DOI: 10.3847/1538-4357/ab12e0 Bibcode: 2019ApJ...876...30S

Menten, Karl M.; Reid, Mark J.; Sakai, Nobuyuki +2 more

We report measurements of parallax and proper motion for five 6.7 GHz methanol maser sources in the outer regions of the Perseus arm as part of the BeSSeL Survey of the Galaxy. By combining our results with previous astrometric results, we determine an average spiral arm pitch angle of 9.°2 ± 1.°5 and an arm width of 0.39 kpc for this spiral arm. …

2019 The Astrophysical Journal
Gaia 21
Signatures of Tidal Disruption in Ultra-faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V
DOI: 10.3847/1538-4357/ab45ec Bibcode: 2019ApJ...885...53M

Caldwell, Nelson; Strader, Jay; Seth, Anil C. +10 more

The ultra-faint dwarf galaxy Leo V has shown both photometric overdensities and kinematic members at large radii, along with a tentative kinematic gradient, suggesting that it may have undergone a close encounter with the Milky Way. We investigate these signs of disruption through a combination of (i) high precision photometry obtained with the Hu…

2019 The Astrophysical Journal
Gaia eHST 21
Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z = 2.26 Galaxy SDSS J0901+1814
DOI: 10.3847/1538-4357/ab22b9 Bibcode: 2019ApJ...879...52S

Wilner, David J.; Keeton, Charles R.; Lutz, Dieter +8 more

We present ∼1″ resolution (∼2 kpc in the source plane) observations of the CO (1-0), CO (3-2), Hα, and [N II] lines in the strongly lensed z = 2.26 star-forming galaxy SDSS J0901+1814. We use these observations to constrain the lensing potential of a foreground group of galaxies, and our source-plane reconstructions indicate that SDSS J0901+1814 i…

2019 The Astrophysical Journal
eHST 21