Search Publications

INTEGRAL View on cataclysmic variables and symbiotic binaries
DOI: 10.1016/j.newar.2020.101547 Bibcode: 2020NewAR..9101547L

Doroshenko, Victor; de Martino, Domitilla; Falanga, Maurizio +5 more

Accreting white dwarfs (WDs) constitute a significant fraction of the hard X-ray sources detected by the INTEGRAL observatory. Most of them are magnetic Cataclysmic Variables (CVs) of the intermediate polar (IP) and polar types, but the contribution of the Nova-likes systems and the systems with optically thin boundary layers, Dwarf Novae (DNs) an…

2020 New Astronomy Reviews
INTEGRAL 14
A census of young stellar population associated with the Herbig Be star HD 200775
DOI: 10.1093/mnras/staa1053 Bibcode: 2020MNRAS.494.5851S

Mathew, Blesson; Manoj, P.; Lee, Chang Won +4 more

The region surrounding the well-known reflection nebula, NGC 7023, illuminated by a Herbig Be star, HD 200775, located in the dark cloud L1174 is studied in this work. Based on the distances and proper motion values from Gaia DR2 of 20 previously known young stellar object (YSO) candidates, we obtained a distance of 335 ± 11 pc to the cloud comple…

2020 Monthly Notices of the Royal Astronomical Society
Gaia Herschel XMM-Newton 14
On the nature of the soft γ-ray emission in the hard state of the black hole transient GRS 1716-249
DOI: 10.1093/mnras/staa739 Bibcode: 2020MNRAS.494..571B

Motta, S. E.; Segreto, A.; Casella, P. +9 more

The black hole transient GRS 1716-249 was monitored from the radio to the γ-ray band during its 2016-2017 outburst. This paper focuses on the spectral energy distribution (SED) obtained in 2017 February-March, when GRS 1716-249 was in a bright hard spectral state. The soft γ-ray data collected with the INTEGRAL/SPI telescope show the presence of a…

2020 Monthly Notices of the Royal Astronomical Society
INTEGRAL 14
A Statistical Search for Star-Planet Interaction in the Ultraviolet Using GALEX
DOI: 10.3847/1538-3881/ab7d3b Bibcode: 2020AJ....159..194V

Mathew, Blesson; Manoj, P.; Kartha, Sreeja S. +2 more

Most (∼82%) of the over 4000 confirmed exoplanets known today orbit very close to their host stars, within 0.5 au. Planets at such small orbital distances can result in significant interactions with their host stars, which can induce increased activity levels in them. In this work, we have searched for statistical evidence for star-planet interact…

2020 The Astronomical Journal
Gaia 14
Magnetohydrodynamic Turbulent Evolution of a Magnetic Cloud in the Outer Heliosphere
DOI: 10.3847/2041-8213/abcb03 Bibcode: 2020ApJ...905L..12T

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +8 more

This Letter exploits joint observations of the same interplanetary coronal mass ejection by widely separated spacecraft to study, for the first time, the turbulent evolution of the magnetohydrodynamic (MHD) properties of the embedded magnetic cloud, during its propagation throughout interplanetary space. Specifically, the event was observed by Win…

2020 The Astrophysical Journal
Ulysses 14
Mirror, mirror on the outflow cavity wall. Near-infrared CO overtone disc emission of the high-mass YSO IRAS 11101-5829
DOI: 10.1051/0004-6361/201936748 Bibcode: 2020A&A...633A.128F

Stecklum, B.; Coffey, D.; Natta, A. +7 more


Aims: The inner regions of high-mass protostars are often invisible in the near-infrared, obscured by thick envelopes and discs. We aim to investigate the inner gaseous disc of IRAS 11101-5829 through scattered light from the outflow cavity walls.
Methods: We observed the immediate environment of the high-mass young stellar object IRAS 1…

2020 Astronomy and Astrophysics
Gaia 14
On the Correlation between L Dwarf Optical and Infrared Variability and Radio Aurorae
DOI: 10.3847/1538-4357/abb826 Bibcode: 2020ApJ...903...74R

Richey-Yowell, Tyler; Kao, Melodie M.; Pineda, J. Sebastian +2 more

Photometric variability attributed to cloud phenomena is common in L/T transition brown dwarfs. Recent studies show that such variability may also trace aurorae, suggesting that localized magnetic heating may contribute to observed brown dwarf photometric variability. We assess this potential correlation with a survey of 17 photometrically variabl…

2020 The Astrophysical Journal
Gaia 14
Observation and Modeling of High-temperature Solar Active Region Emission during the High-resolution Coronal Imager Flight of 2018 May 29
DOI: 10.3847/1538-4357/ab917c Bibcode: 2020ApJ...896...51W

Golub, Leon; Winebarger, Amy R.; Warren, Harry P. +15 more

Excellent coordinated observations of NOAA active region 12712 were obtained during the flight of the High-resolution Coronal Imager (Hi-C) sounding rocket on 2018 May 29. This region displayed a typical active region core structure with relatively short, high-temperature loops crossing the polarity inversion line and bright "moss" located at the …

2020 The Astrophysical Journal
Hinode IRIS 14
Evidence of Particle Acceleration in the Superbubble 30 Doradus C with NuSTAR
DOI: 10.3847/1538-4357/ab8232 Bibcode: 2020ApJ...893..144L

Auchettl, Katie; Madsen, Kristin K.; Grefenstette, Brian W. +2 more

We present evidence of diffuse, non-thermal X-ray emission from the superbubble 30 Doradus C (30 Dor C) using hard X-ray images and spectra from NuSTAR observations. For this analysis, we utilize data from a 200 ks targeted observation of 30 Dor C as well as 2.8 Ms of serendipitous off-axis observations from the monitoring of nearby SN 1987A. The …

2020 The Astrophysical Journal
XMM-Newton 14
The observational impact of dust trapping in self-gravitating discs
DOI: 10.1093/mnras/staa2596 Bibcode: 2020MNRAS.498.4256C

Cadman, James; Hall, Cassandra; Rice, Ken +2 more

We present a 3D semi-analytical model of self-gravitating discs, and include a prescription for dust trapping in the disc spiral arms. Using Monte Carlo radiative transfer, we produce synthetic ALMA (Atacama Large Millimeter/submillimeter Array) observations of these discs. In doing so, we demonstrate that our model is capable of producing observa…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 14