Search Publications

AG Leonis Minoris-An evolved, detached eclipsing binary
DOI: 10.1016/j.newast.2020.101362 Bibcode: 2020NewA...7701362N

Nelson, Robert H.

Radial velocity data and photometric light curves (in the B. V, and Ic passbands) for the detached eclipsing binary AG Leo Minoris were acquired-apparently for the first time-and are reported here. Roche modelling using the 2003 version of the Wilson-Devinney code was completed, yielding the basic parameters. The period appears to be co…

2020 New Astronomy
Gaia 3
A Test of Gravitational Theories Including Torsion with the BepiColombo Radio Science Experiment
DOI: 10.3390/universe6100175 Bibcode: 2020Univ....6..175S

Schettino, Giulia; Serra, Daniele; Tommei, Giacomo +1 more

Within the framework of the relativity experiment of the ESA/JAXA BepiColombo mission to Mercury, which was launched at the end of 2018, we describe how a test of alternative theories of gravity, including torsion can be set up. Following March et al. (2011), the effects of a non-vanishing spacetime torsion have been parameterized by three torsion…

2020 Universe
BepiColombo 3
HST/FGS Trigonometric Parallaxes of M-dwarf Eclipsing Binaries
DOI: 10.1088/1538-3873/ab7b91 Bibcode: 2020PASP..132e4201V

Schaefer, Gail H.; Nelan, Edmund P.; Ciardi, David R. +5 more

Hubble Space Telescope (HST) Fine Guidance Sensor (FGS) trigonometric parallax observations were obtained to directly determine distances to five nearby M-dwarf/M-dwarf eclipsing binary systems. These systems are intrinsically interesting as benchmark systems for establishing basic physical parameters for low-mass stars, such as luminosity L, and …

2020 Publications of the Astronomical Society of the Pacific
Gaia eHST 3
Environmental Impact on Star-forming Galaxies in a z ∼ 0.9 Cluster during the Course of Galaxy Accretion
DOI: 10.3847/1538-4357/ab9dfb Bibcode: 2020ApJ...899...64A

Suzuki, Tomoko L.; Koyama, Yusei; Kodama, Tadayuki +18 more

Galaxies change their properties as they assemble into clusters. In order to understand the physics behind that, we need to go back in time and observe directly what is occurring in galaxies as they fall into a cluster. We have conducted a narrowband and J-band imaging survey on a cluster CL1604-D at z = 0.923 using a new infrared instrument SWIMS…

2020 The Astrophysical Journal
eHST 3
Multiwavelength Imaging and Spectral Analysis of Jet-like Phenomena in a Solar Active Region Using IRIS and AIA
DOI: 10.3847/1538-4357/ab974d Bibcode: 2020ApJ...898...17H

Morgan, Huw; Humphries, Llŷr Dafydd; Verwichte, Erwin +1 more

High-resolution observations of dynamic phenomena give insights into the properties and processes that govern the low solar atmosphere. We present an analysis of jet-like phenomena emanating from a penumbral footpoint in active region (AR) 12192 using imaging and spectral observations from the Interface Region Imaging Spectrograph (IRIS) and the A…

2020 The Astrophysical Journal
IRIS 3
The Nature of the Double Nuclei in the Barred S0 Galaxy IC 676
DOI: 10.3847/1538-4357/ab6f02 Bibcode: 2020ApJ...890..145Z

Zhou, Xu; Ma, Jun; Zhou, Zhimin +1 more

The lenticular galaxy IC 676 is a barred galaxy with double nuclei and active star formation in the central region. In this work we present the long-slit spectroscopy and archival multiwavelength images to investigate the nature and origin of the double nuclei in IC 676. Through photometric 1D brightness profiles and 2D image decomposition, we sho…

2020 The Astrophysical Journal
eHST 3
Guide star catalog generation of star sensors for interstellar navigation
DOI: 10.1117/1.JATIS.6.4.044006 Bibcode: 2020JATIS...6d4006W

Wu, Liang

In interstellar travel, parallax and stellar aberration have a non-negligible influence on the star identification of star sensors. Through the analysis of the working principle of star sensors, only the guide star catalog generation can solve this problem. The influence mechanism of parallax and stellar aberration is synthetically analyzed by fou…

2020 Journal of Astronomical Telescopes, Instruments, and Systems
Hipparcos 3
Solar-cycle-related Changes in the Helium Ionization Zones of the Sun
DOI: 10.3847/2041-8213/abc348 Bibcode: 2020ApJ...903L..29W

Basu, Sarbani; Watson, Courtney B.

Helioseismic data for solar cycles 23 and 24 have shown unequivocally that solar dynamics changes with solar activity. Changes in solar structure have been more difficult to detect. Basu & Mandel had claimed that the then-available data revealed changes in the He II ionization zone of the Sun. The amount of change, however, indicated the need …

2020 The Astrophysical Journal
SOHO 3
Understanding the Structure of Rapid Intensity Fluctuations in the Chromosphere with IRIS
DOI: 10.3847/1538-4357/ab5f6b Bibcode: 2020ApJ...889..112S

De Pontieu, B.; Schmit, D.; Winebarger, A. +2 more

Several recent data sets have taken advantage of the unique capabilities of orbital and suborbital spacecraft to image the chromosphere and transition region at a very high cadence. We find that both the chromosphere and transition region exhibit spatially coherent transient features at frequencies above 80 mHz. We have analyzed narrowband imaging…

2020 The Astrophysical Journal
IRIS 3
Doppler shifts and spectral line profile changes in the starlight scattered from an exoplanet
DOI: 10.1093/mnras/staa268 Bibcode: 2020MNRAS.493.1596S

Anglada-Escudé, Guillem; Strachan, John B. P.

Scattered starlight from an exoplanet, commonly called reflected light, can be used to characterize the planet including the determination of its albedo and inclination of orbit. The relatively low flux ratio between directly observed starlight and starlight scattered off hot Jupiters make these systems the prime candidates for detection of reflec…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 3