Search Publications

Characterising young visual M-dwarf binaries with near-infrared integral field spectra
DOI: 10.1051/0004-6361/202038030 Bibcode: 2020A&A...642A..57C

Calissendorff, Per; Janson, Markus; Bonnefoy, Mickaël

We present the results from an integral field spectroscopy study of seven close visual binary pairs of young M-dwarf multiple systems. The target systems are part of the astrometric monitoring AstraLux programme, surveying hundreds of M-dwarf systems for multiplicity and obtaining astrometric epochs for orbital constraints. Our new VLT/SINFONI dat…

2020 Astronomy and Astrophysics
Gaia 3
On the correctness of orbital solutions obtained from a small set of points. Orbit of HIP 53731
DOI: 10.1088/1674-4527/20/11/187 Bibcode: 2020RAA....20..187M

Mitrofanova, Arina; Dyachenko, Vladimir; Beskakotov, Anatoly +4 more

HIP 53731 is a binary consisting of stars of the spectral types K0 and K9. The orbit of this object was constructed previously by Cvetković et al. and improved by Tokovinin. It should be noted that there is a 180° ambiguity in the position angles of some published measurements. Speckle interferometric observations were obtained in 2007-2020 (21 me…

2020 Research in Astronomy and Astrophysics
Gaia Hipparcos 3
Radio Sounding Measurements of the Solar Corona Using Giant Pulses of the Crab Pulsar in 2018
DOI: 10.1007/s11207-020-01644-w Bibcode: 2020SoPh..295...80T

Tokumaru, Munetoshi; Terasawa, Toshio; Sekido, Mamoru +2 more

Observations of the Crab pulsar at 327 MHz were made at the Toyokawa Observatory of the Institute for Space-Earth Environmental Research, during the solar occultation in mid-June 2018 to investigate the coronal plasma density in the weak sunspot cycle, Cycle 24. The dispersion measurements (DMs) were determined using giant pulses detected from obs…

2020 Solar Physics
SOHO 3
Kepler Binary Stars in the NGC 6819 Open Cluster: KIC 5113146 and KIC 5111815
DOI: 10.3847/1538-3881/abbb35 Bibcode: 2020AJ....160..245S

Bilir, Selçuk; Soydugan, Faruk; Soydugan, Esin +1 more

In this study, an investigation of two double-lined binary stars KIC 5113146 and KIC 5111815 in the NGC 6819 open cluster is presented based on both photometric and spectroscopic data. Simultaneous analysis of light and radial velocity curves was made and the absolute parameters of the systems' components were determined for the first time. We fin…

2020 The Astronomical Journal
Gaia 3
Discovery of recombining plasma associated with the candidate supernova remnant G189.6+3.3 with Suzaku
DOI: 10.1093/pasj/psaa070 Bibcode: 2020PASJ...72...81Y

Nobukawa, Kumiko K.; Yamauchi, Shigeo; Pannuti, Thomas G. +1 more

We present the results of an X-ray spectral analysis of the northeast region of the candidate supernova remnant G189.6+3.3 with Suzaku. K-shell lines from highly ionized Ne, Mg, Si, and S were detected in the spectrum for the first time. In addition, a radiative recombining continuum (RRC) from He-like Si was clearly seen near 2.5 keV. This detect…

2020 Publications of the Astronomical Society of Japan
Suzaku 3
Seasonal thermal inertia variations at Gale crater: Role of active surface deposition phenomena
DOI: 10.1016/j.icarus.2019.113499 Bibcode: 2020Icar..33713499R

Rangarajan, Vidhya Ganesh; Ghosh, Mili

Thermal inertia has been found to play a significant role in planetary remote sensing applications, forming the basis of potentially all major lithological discriminations of the planetary surface. It has always been visualised to serve as a distinctive thermal property of the surface with its values remaining fairly constant at least for a short …

2020 Icarus
MEx 3
ASAS census of twins
DOI: 10.1093/mnras/staa1587 Bibcode: 2020MNRAS.496.2605B

Bakış, Volkan; Yücel, Gökhan; Eker, Zeki +2 more

Twin binaries were identified among the eclipsing binaries with δ > -30° listed in the All Sky Automated Survey (ASAS) catalogue. In addition to the known twin binaries in the literature, 68 new systems have been identified and photometric and spectroscopic observations were done. Colour, spectral type, temperature, ratio of radii and masses of…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 3
A Large Massive Quiescent Galaxy Sample at z ∼ 1.2
DOI: 10.3847/1538-4357/abbeff Bibcode: 2020ApJ...905..103X

Sawicki, Marcin; Cheng, Cheng; Huang, Jia-Sheng +8 more

In this paper we present a simple color-magnitude selection and obtain a large sample of 33,893 massive quiescent galaxies at intermediate redshifts (1 < z < 1.5). We choose the longest wavelength available in the Hyper-Supreme-Cam (HSC) deep survey, the Y band and i - Y color, to select the 4000 Å Balmer jump in passive galaxies to the high…

2020 The Astrophysical Journal
eHST 3
The effects of unresolved double degenerates in the white dwarf luminosity function
DOI: 10.1093/mnras/stz3371 Bibcode: 2020MNRAS.491.5671R

Rebassa-Mansergas, A.; Torres, S.; Toonen, S. +1 more

We perform an analysis of the single white dwarf and the double degenerate binary populations in the solar neighbourhood following a population synthesis approach to investigate the effects of unresolved double degenerates in the white dwarf luminosity function. We consider all unresolved synthetic binaries to be associated with fictitious effecti…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 3
Variability of the Great Disk Shadow in Serpens
DOI: 10.3847/1538-4357/ab91ae Bibcode: 2020ApJ...896..169P

Green, Joel D.; Pontoppidan, Klaus M.; Salyk, Colette +2 more

We present dual-epoch Hubble Space Telescope imaging of the great disk shadow in the Serpens star-forming region. The near-infrared images show strong variability of the disk shadow, revealing dynamics of the inner disk on timescales of months. The Great Shadow is projected onto the Serpens reflection nebula by an unresolved protoplanetary disk su…

2020 The Astrophysical Journal
Herschel eHST 3