Search Publications

An extreme ultraluminous X-ray source X-1 in NGC 5055
DOI: 10.1051/0004-6361/202038684 Bibcode: 2020A&A...642A..94M

Mondal, Samaresh; De Marco, Barbara; Różańska, Agata +1 more


Aims: We analysed multi-epoch X-ray data of the ultraluminous X-ray source NGC 5055 X-1, with luminosity up to 2.32 × 1040 erg s-1, to constrain the physical parameters of the source.
Methods: We performed a timing and spectral analysis of Chandra and XMM-Newton observations. We used spectral models that assume the …

2020 Astronomy and Astrophysics
XMM-Newton 5
Unusually low density regions in the compressed slow wind: Solar wind transients of small coronal hole origin
DOI: 10.1051/0004-6361/201935884 Bibcode: 2020A&A...635A..49L

Farrugia, Charles J.; Wang, Linghua; Fu, Hui +5 more

We report on two small solar wind transients embedded in the corotating interaction region, characterized by surprisingly lower proton density compared with their surrounding regions. In addition to lower density, these two small solar wind transients showed other interesting features like higher proton temperature, higher alpha-proton ratios, and…

2020 Astronomy and Astrophysics
SOHO 5
The Wind beneath My Wings. I. Spectral Types and Multiplicity of the Central Stars Supporting Stellar Bow Shock Nebulae
DOI: 10.3847/1538-4365/abc0e5 Bibcode: 2020ApJS..251...29C

Kobulnicky, Henry A.; Dixon, Don M.; Schurhammer, Danielle P. +9 more

Arcuate mid-infrared nebulae known as stellar bow shock nebulae (SBNe) have been previously hypothesized to be supported by the strong stellar winds and/or luminosity of massive early-type stars. We present an optical spectroscopic survey of 84 stars identified from mid-infrared images as candidate SBN-supporting stars. Eighty-one of 84 sources, 9…

2020 The Astrophysical Journal Supplement Series
Gaia 5
XMM-Newton and NICER Measurement of the Rms Spectrum of the Millihertz Quasiperiodic Oscillations in the Neutron-star Low-mass X-Ray Binary 4U 1636-53
DOI: 10.3847/1538-4357/ab8cbe Bibcode: 2020ApJ...895..120L

Altamirano, D.; Méndez, Mariano; Zhang, Guobao +4 more

We used two XMM-Newton and six Neutron Star Interior Composition Explorer observations to investigate the fractional rms amplitude of the millihertz quasiperiodic oscillations (mHz QPOs) in the neutron-star low-mass X-ray binary 4U 1636-53. We studied, for the first time, the fractional rms amplitude of the mHz QPOs versus energy in 4U 1636-53 dow…

2020 The Astrophysical Journal
XMM-Newton 5
Search for the optical counterpart of the GW170814 gravitational wave event with the VLT Survey Telescope
DOI: 10.1093/mnras/stz3536 Bibcode: 2020MNRAS.492.1731G

Covino, S.; Campana, S.; Della Valle, M. +30 more

We report on the search for the optical counterpart of the gravitational event GW170814, which was carried out with the VLT Survey Telescope (VST) by the GRAvitational Wave Inaf TeAm. Observations started 17.5 h after the Laser Interferometer Gravitational-wave Observatory (LIGO) and Virgo alert and we covered an area of 99 deg2 that en…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 5
Evolving pulsation of the slowly rotating magnetic β Cep star ξ1 CMa
DOI: 10.1093/mnras/staa025 Bibcode: 2020MNRAS.492.2762W

Handler, G.; Wade, G. A.; Pigulski, A. +11 more

Recent BRITE-Constellation space photometry of the slowly rotating, magnetic β Cep pulsator ξ1 CMa permits a new analysis of its pulsation properties. Analysis of the two-colour BRITE data reveals the well-known single pulsation period of 0.209 d, along with its first and second harmonics. A similar analysis of SMEI and TESS observation…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 5
Disturbed Flows in the Inner Solar Wind and Near Earth's Orbit
DOI: 10.1134/S0010952519060029 Bibcode: 2020CosRe..57..423E

Pätzold, M.; Bird, M. K.; Efimov, A. I. +3 more

Coronal mass ejections from active regions on the Sun can be observed as series of individual events separated in time in the inner solar wind and near-Earth plasma. To find such events we have analyzed experimental data of dual-frequency solar wind radio sounding by the Rosetta and Mars Express spacecraft. The cycles of experiments performed in 2…

2020 Cosmic Research
Rosetta SOHO 5
A white dwarf bound to the transiting planetary system WASP-98
DOI: 10.1093/mnras/staa2328 Bibcode: 2020MNRAS.497.4416S

Gänsicke, Boris T.; Močnik, Teo; Tremblay, Pier-Emmanuel +2 more

WASP-98 is a planetary system containing a hot Jupiter transiting a late-G dwarf. A fainter star, 12 arcsec away, has previously been identified as a white dwarf, with a distance and proper motion consistent with a physical association with the planetary system. We present spectroscopy of the white dwarf, with the aim of determining its mass, radi…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 5
A search for pulsars in subdwarf B binary systems and discovery of giant-pulse emitting PSR J0533-4524
DOI: 10.1093/mnras/staa146 Bibcode: 2020MNRAS.492.4825O

Ishwara-Chandra, C. H.; van Leeuwen, J.; Coenen, T. +2 more

Binary millisecond pulsars (MSPs) provide several opportunities for research of fundamental physics. However, finding them can be challenging. Several subdwarf B (sdB) binary systems with possible neutron star companions have been identified, allowing us to perform a targeted search for MSPs within these systems. Six sdBs with companions in the ne…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 5
Simple, compact, high-resolution monochromatic x-ray source for characterization of x-ray calorimeter arrays
DOI: 10.1063/5.0005206 Bibcode: 2020RScI...91h3110L

Eckart, M. E.; Kilbourne, C. A.; Leutenegger, M. A. +6 more

X-ray calorimeters routinely achieve very high spectral resolution, typically a few eV full width at half maximum (FWHM). Measurements of calorimeter line shapes are usually dominated by the natural linewidth of most laboratory calibration sources. This compounds the data acquisition time necessary to statistically sample the instrumental line bro…

2020 Review of Scientific Instruments
Hitomi 5