Search Publications

Unusual Isotopic Abundances in a Fully Convective Stellar Binary
DOI: 10.3847/2041-8213/aaf9b6 Bibcode: 2019ApJ...871L...3C

Mills, E. A. C.; Crossfield, I. J. M.; Lothringer, J. D. +6 more

Low-mass M dwarfs represent the most common outcome of star formation, but their complex emergent spectra hinder detailed studies of their composition and initial formation. The measurement of isotopic ratios is a key tool that has been used to unlock the formation of our solar system, the Sun, and the nuclear processes within more massive stars. …

2019 The Astrophysical Journal
Gaia 16
The Duration of Star Formation in Galactic Giant Molecular Clouds. I. The Great Nebula in Carina
DOI: 10.3847/1538-4357/ab26b2 Bibcode: 2019ApJ...881...37P

Povich, Matthew S.; Nuñez, Evan Haze; Robitaille, Thomas P. +1 more

We present a novel infrared spectral energy distribution (SED) modeling methodology that uses likelihood-based weighting of the model fitting results to construct probabilistic Hertzsprung-Russell diagrams (pHRD) for X-ray-identified, intermediate-mass (2-8 M ), pre-main-sequence young stellar populations. This methodology is designed …

2019 The Astrophysical Journal
Gaia 16
High-fidelity Imaging of the Inner AU Mic Debris Disk: Evidence of Differential Wind Sculpting?
DOI: 10.3847/2041-8213/ab40bf Bibcode: 2019ApJ...883L...8W

Stark, Christopher C.; Kowalski, Adam F.; Davenport, James R. A. +17 more

We present new high-fidelity optical coronagraphic imagery of the inner ∼50 au of AU Mic’s edge-on debris disk using the BAR5 occulter of the Hubble Space Telescope Imaging Spectrograph (HST/STIS) obtained on 2018 July 26-27. This new imagery reveals that “feature A,” residing at a projected stellocentric separation of 14.2 au on the southeast sid…

2019 The Astrophysical Journal
Gaia eHST 16
Hubble Space Telescope Emission-line Images of Nearby 3CR Radio Galaxies: Two Photoionization, Accretion, and Feedback Modes
DOI: 10.3847/1538-4357/aaf002 Bibcode: 2019ApJ...870...53B

Sparks, William B.; Chiaberge, Marco; Capetti, Alessandro +3 more

We present HST/ACS narrowband images of a low-z sample of 19 3C radio galaxies to study the Hα and [O III] emissions from the narrow-line region. Based on nuclear emission-line ratios, we divide the sample into high- and low-excitation galaxies (HEGs and LEGs). We observe different line morphologies, extended [O III] emission, large [O III]/Hα sca…

2019 The Astrophysical Journal
eHST 16
A Search for Water Vapor Plumes on Europa using SOFIA
DOI: 10.3847/2041-8213/aafb0a Bibcode: 2019ApJ...871L...5S

Sparks, W. B.; Dello Russo, N.; Hand, K. P. +8 more

We present mid-infrared Stratospheric Observatory for Infrared Astronomy (SOFIA)/Echelon Cross Echelle Spectrograph (EXES) spectroscopy of Europa, seeking direct evidence of the presence of water vapor arising from plumes venting from the surface. We place quantitatively useful upper limits on the strength of water vibrational-rotational emission …

2019 The Astrophysical Journal
eHST 16
Genus Statistic Applied to the X-Ray Remnant of SN 1572: Clues to the Clumpy Ejecta Structure of Type Ia Supernovae
DOI: 10.3847/1538-4357/ab24db Bibcode: 2019ApJ...879...64S

Sato, Toshiki; Hughes, John P.; Williams, Brian J. +1 more

Clumpy structures are a common feature in X-ray images of young Type Ia supernova remnants (SNRs). Although the precise origin of such clumps remains unclear, there are three generic possibilities: clumpiness imposed during the explosion, hydrodynamic instabilities that act during the remnant’s evolution, and preexisting structures in the ambient …

2019 The Astrophysical Journal
XMM-Newton 15
A Comparison of the X-Ray Properties of FU Ori-type Stars to Generic Young Stellar Objects
DOI: 10.3847/1538-4357/ab3a3f Bibcode: 2019ApJ...883..117K

Hillenbrand, Lynne A.; Kuhn, Michael A.

Like other young stellar objects (YSOs), FU Ori-type stars have been detected as strong X-ray emitters. However, little is known about how the outbursts of these stars affect their X-ray properties. We assemble available X-ray data from XMM-Newton and Chandra observations of 16 FU Ori stars, including a new XMM-Newton observation of Gaia 17bpi dur…

2019 The Astrophysical Journal
Gaia XMM-Newton 15
Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
DOI: 10.3847/1538-4357/ab4269 Bibcode: 2019ApJ...884...67W

Whitten, Devin D.; Beers, Timothy C.; Placco, Vinicius M. +6 more

We present an analysis of the relative age distribution of the Milky Way halo, based on samples of blue horizontal-branch (BHB) stars obtained from the Panoramic Survey Telescope and Rapid Response System and Galaxy Evolution Explorer photometry, as well a Sloan Digital Sky Survey spectroscopic sample. A machine-learning approach to the selection …

2019 The Astrophysical Journal
Gaia 15
TOI-150: A Transiting Hot Jupiter in the TESS Southern CVZ
DOI: 10.3847/2041-8213/ab21c0 Bibcode: 2019ApJ...877L..29C

Butler, R. Paul; Schneider, Donald P.; Kollmeier, Juna A. +24 more

We report the detection of a hot Jupiter ({M}p={1.75}-0.17+0.14 {M}{{J}}, R p = 1.38 ± 0.04 R J) orbiting a middle-aged star ({log}g={4.152}-0.043+0.030) in the Transiting Exoplanet Survey Satellite (TESS) southern continuous viewing zone (β = -79.°59). We co…

2019 The Astrophysical Journal
Gaia 15
A BCG with Offset Cooling: Is the AGN Feedback Cycle Broken in A2495?
DOI: 10.3847/1538-4357/ab4808 Bibcode: 2019ApJ...885..111P

Gastaldello, F.; Ettori, S.; Amblard, A. +6 more

We present a combined radio/X-ray analysis of the poorly studied galaxy cluster A2495 (z = 0.07923) based on new EVLA and Chandra data. We also analyze and discuss Hα emission and optical continuum data retrieved from the literature. We find an offset of ∼6 kpc between the cluster brightest cluster galaxy (BCG) (MCG+02-58-021) and the peak of the …

2019 The Astrophysical Journal
eHST 15