Search Publications

Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur Revisited
DOI: 10.3847/1538-4357/ab43e5 Bibcode: 2019ApJ...885..105R

Rangelov, Blagoy; Federman, S. R.; Montmerle, Thierry +2 more

We present results of our Chandra/ACIS observations of the field centered on the fast, runaway O star AE Aur and its bow shock. Previous XMM-Newton observations revealed an X-ray “blob” near the IR arc tracing the bow shock, possibly a nonthermal source consistent with models of Inverse Compton scattering of dust IR photons by electrons accelerate…

2019 The Astrophysical Journal
XMM-Newton 6
Spectroscopy of NGC 4258 Globular Cluster Candidates: Membership Confirmation and Kinematics
DOI: 10.3847/1538-4357/ab113a Bibcode: 2019ApJ...876...39G

González-Lópezlira, Rosa A.; Georgiev, Iskren Y.; Loinard, Laurent +9 more

We present multiobject spectroscopic observations of 23 globular cluster candidates (GCCs) in the prototypical megamaser galaxy NGC 4258, carried out with the Optical System for Imaging and low-Intermediate-Resolution Integrated Spectroscopy instrument at the 10.4 m Gran Telescopio Canarias. The candidates have been selected based on the (u* - i‧)…

2019 The Astrophysical Journal
eHST 6
The Next Generation Fornax Survey (NGFS). V. Discovery of a Dwarf-Dwarf Galaxy Pair at z = 0.30 and Its Characterization Using Deep VLT/MUSE Observations
DOI: 10.3847/1538-4357/ab0419 Bibcode: 2019ApJ...873...59J

Grebel, Eva K.; Mieske, Steffen; Rong, Yu +11 more

We report the detection of a pair of dwarf galaxies at z = 0.30 that may be in the early stages of an interaction. Both galaxies have stellar masses of <109 M and display a projected separation of ∼29 kpc and a physical separation of ∼240 kpc. Evidence of ongoing star formation has been found in both galaxies, with neith…

2019 The Astrophysical Journal
eHST 6
The Origins of Young Stars in the Direction of the Leading Arm of the Magellanic Stream: Abundances, Kinematics, and Orbits
DOI: 10.3847/1538-4357/aaf560 Bibcode: 2019ApJ...871...99Z

Zhao, Gang; Casetti-Dinescu, Dana I.; Girard, Terrence M. +6 more

We explore the origins of the young B-type stars found by Casetti-Dinescu et al. at the outskirts of the Milky Way disk in the sky region of the Leading Arm of the Magellanic Stream. High-resolution spectroscopic observations made with the MIKE instrument on the Magellan Clay 6.5 m telescope for nine stars are added to the previous sample analyzed…

2019 The Astrophysical Journal
Gaia 6
Dissecting the Hot Bubbles in LMC-N57 with XMM-Newton
DOI: 10.3847/1538-4357/ab44cf Bibcode: 2019ApJ...885..116R

Toalá, Jesús A.; Rosado, Margarita; Ramírez-Ballinas, Isidro +1 more

We present a study of the diffuse X-ray emission from the star-forming region LMC-N 57 in the Large Magellanic Cloud. We use archival XMM-Newton observations to unveil in detail the distribution of hot bubbles in this complex. X-ray emission is detected from the central superbubble (SB) DEM L 229, the supernova remnant (SNR) 0532-675, and the Wolf…

2019 The Astrophysical Journal
XMM-Newton 6
X-Ray Monitoring of the Magnetar CXOU J171405.7-381031 in Supernova Remnant CTB 37B
DOI: 10.3847/1538-4357/ab378c Bibcode: 2019ApJ...882..173G

Gotthelf, E. V.; Halpern, J. P.; Mori, K. +1 more

We present the results of our 8 yr X-ray monitoring campaign on CXOU J171405.7-381031, the magnetar associated with the faint supernova remnant (SNR) CTB 37B. It is among the youngest by inferred spin-down age, and most energetic in spin-down power of magnetars, and may contribute, at least partially, to the GeV and TeV emission coincident with th…

2019 The Astrophysical Journal
XMM-Newton 6
Smoothed Particle Inference Analysis of SNR DEM L71
DOI: 10.3847/1538-4357/ab0e81 Bibcode: 2019ApJ...875...14F

Frank, Kari A.; Burrows, David N.; Panfichi, Aldo +2 more

Supernova remnants (SNRs) are complex, three-dimensional objects; properly accounting for this complexity when modeling the resulting X-ray emission presents quite a challenge and makes it difficult to accurately characterize the properties of the full SNR volume. We apply for the first time a novel analysis method called smoothed particle inferen…

2019 The Astrophysical Journal
XMM-Newton 6
Quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR Observations of the New X-Ray Clocked Burster 1RXS J180408.9-342058
DOI: 10.3847/1538-4357/ab4d59 Bibcode: 2019ApJ...887...30F

Fiocchi, M.; Ubertini, P.; Bazzano, A. +4 more

We report the quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR observations showing spectral state transitions in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 during its 2015 outburst. We present results of the analysis of high-quality broad energy band (0.8-200 keV) data in three different spectral states: high/soft, low/very-hard, …

2019 The Astrophysical Journal
INTEGRAL 6
A Supernova Remnant Counterpart for HESS J1832-085
DOI: 10.3847/1538-4357/ab3e3f Bibcode: 2019ApJ...885..129M

Haberl, F.; Filipović, M. D.; Pühlhofer, G. +18 more

We examine the new Galactic supernova remnant (SNR) candidate, G23.11+0.18, as seen by the Murchison Widefield Array radio telescope. We describe the morphology of the candidate and find a spectral index of -0.63 ± 0.05 in the 70-170 MHz domain. Coincident TeV gamma-ray detection in High Energy Stereoscopic System (HESS) data supports the SNR natu…

2019 The Astrophysical Journal
XMM-Newton 6
A New Einstein Cross Gravitational Lens of a Lyman-break Galaxy
DOI: 10.3847/2041-8213/ab0aeb Bibcode: 2019ApJ...873L..14B

Corradi, Romano L. M.; Vulcani, Benedetta; Negrello, Mattia +5 more

We report the study of an “Einstein Cross” configuration first identified in a set of HST images by Cerny et al. Deep spectroscopic observations obtained at the Spanish 10.4 m Gran Telescopio Canarias telescope, allowed us to demonstrate the lens nature of the system, that consists of a Lyman-break galaxy (LBG), not a quasi-stellar object as is us…

2019 The Astrophysical Journal
eHST 6