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
Cassini UVIS Detection of Saturn's North Polar Hexagon in the Grand Finale Orbits
DOI: 10.1029/2019JE005922 Bibcode: 2019JGRE..124.1979P

Lamy, L.; West, R. A.; Esposito, L. W. +6 more

Cassini's final orbits in 2016 and 2017 provided unprecedented spatial resolution of Saturn's polar regions from near-polar spacecraft viewing geometries. Long-wavelength channels of Cassini's Ultraviolet Imaging Spectrograph instrument detected Saturn's UV-dark north polar hexagon near 180 nm at planetocentric latitudes near 75°N. The dark polar …

2019 Journal of Geophysical Research (Planets)
Cassini 6
X-ray and radio studies of SNR CTB 37B hosting the magnetar CXOU J171405.7-381031
DOI: 10.1093/mnras/stz1656 Bibcode: 2019MNRAS.487.5019B

Safi-Harb, Samar; Kothes, Roland; Gotthelf, Eric V. +2 more

We present a Chandra and XMM-Newton study of the supernova remnant (SNR) CTB 37B, along with archival radio observations. In radio wavelengths, the SNR CTB 37B is an incomplete shell showing bright emission from the eastern side, while the X-ray morphology shows diffuse emission from regions surrounding the magnetar CXOU J171405.7-381031. We used …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
Multifractal detrended moving average analysis of Kepler stars with surface differential rotation traces
DOI: 10.1093/mnras/stz1791 Bibcode: 2019MNRAS.488.3274D

De Medeiros, J. R.; de Freitas, D. B.; Das Chagas, M. L. +2 more

A multifractal formalism is employed to analyse high-precision time-series data of Kepler stars with surface differential rotation (DR) traces. The multifractal detrended moving average (MFDMA) algorithm has been explored to characterize the multiscale behaviour of the observed time series from a sample of 662 stars selected with parameters close …

2019 Monthly Notices of the Royal Astronomical Society
SOHO 6
Detection of Hα emission from PZ Telescopii B using SPHERE/ZIMPOL
DOI: 10.1051/0004-6361/201936510 Bibcode: 2019A&A...631A..84M

Henning, Thomas; Musso Barcucci, Arianna; Launhardt, Ralf +6 more

Hα is a powerful tracer of accretion and chromospheric activity, which has been detected in the case of young brown dwarfs and even recently in planetary mass companions (e.g. PDS70 b and c). Hα detections and characterisation of brown dwarf and planet companions can further our knowledge of their formation and evolution, and expanding such a samp…

2019 Astronomy and Astrophysics
Gaia 6
SN 2016B a.k.a. ASASSN-16ab: a transitional Type II supernova
DOI: 10.1093/mnras/stz949 Bibcode: 2019MNRAS.486.2850D

Pandey, S. B.; Benetti, S.; Kumar, Brajesh +12 more

We present photometry, polarimetry, and spectroscopy of the Type II supernova ASASSN-16ab/SN 2016B in PGC 037392. The photometric and spectroscopic follow-up commenced about 2 weeks after shock breakout and continued until nearly 6 months. The light curve of SN 2016B exhibits intermediate properties between those of Type IIP and IIL. The early dec…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6
Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
DOI: 10.1051/0004-6361/201834159 Bibcode: 2019A&A...621A..25F

Rosado, M.; Amram, P.; Fuentes-Carrera, I. +6 more

Context. Encounters between galaxies modify their morphology, kinematics, and star formation history. The relation between these changes and external perturbations is not straightforward. The great number of parameters involved requires both the study of large samples and individual encounters where particular features, motions, and perturbations …

2019 Astronomy and Astrophysics
eHST 6
On ancient solar-type stars
DOI: 10.1093/mnras/sty2660 Bibcode: 2019MNRAS.482..471F

Fuhrmann, Klaus; Chini, Rolf

We describe a survey of ancient solar-type stars down to main-sequence effective temperatures Teff ≥ 5300 K and within 42 pc of the Sun. The underlying Gaia-based, volume-complete parent sample consists of 1633 sources, dominated by Population I. The design of the survey is such that around 130 sources are expected to be members of Popu…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6
Acceleration of plasma in current sheet during substorm dipolarizations in the Earth's magnetotail: Comparison of different mechanisms
DOI: 10.1063/1.5082715 Bibcode: 2019PhPl...26d2901P

Parkhomenko, Elena I.; Malova, Helmi V.; Grigorenko, Elena E. +6 more

This work is devoted to the investigation of particle acceleration during magnetospheric dipolarizations. A numerical model is presented taking into account the four scenarios of plasma acceleration that can be realized: (A) total dipolarization with characteristic time scales of ≈3 min; (B) single peak value of the normal magnetic component

2019 Physics of Plasmas
Cluster 6