Search Publications

Census of Variable Stars toward Serpens Main
DOI: 10.3847/1538-3881/abfdcd Bibcode: 2021AJ....162...52Y

Chen, Zhiwei; Li, Yao; Haas, Martin +7 more

We monitored a 3 deg2 area toward Serpens Main in the Pan-STARRS1 r, i, and z bands from 2016 April to September. Light curves of more than 11,000 stars in each band were obtained, and 143 variables have been identified. Among those, 119 variables are new discoveries, while 24 variables were previously known. We present variability clas…

2021 The Astronomical Journal
Gaia 2
Magnetic flux structuring of the quiet Sun internetwork. Center-to-limb analysis of solar-cycle variations
DOI: 10.1051/0004-6361/202140705 Bibcode: 2021A&A...651A..21F

Faurobert, M.; Ricort, G.

Context. The small-scale magnetism of the quiet Sun has been investigated by various means in recent decades. It is now well established that the quiet Sun contains in total more magnetic flux than active regions and represents an important reservoir of magnetic energy. But the nature and evolution of these fields remain largely unknown.
Aims…

2021 Astronomy and Astrophysics
Hinode 2
VZ Sex: X-Ray Confirmation of Its Intermediate Polar Nature
DOI: 10.3847/1538-4357/abc7ca Bibcode: 2021ApJ...906..134N

Nucita, A. A.; De Paolis, F.; Ingrosso, G. +3 more

Intermediate polars are members of the cataclysmic variable binary stars. They are characterized by a moderately magnetized white dwarf accreting matter from a cool main-sequence companion star. In many cases, this accretion gives rise to a detectable X-ray emission. VZ Sex is an interesting X-ray source whose nature needs a robust confirmation. H…

2021 The Astrophysical Journal
Gaia XMM-Newton 2
Searching for Low-mass Population III Stars Disguised as White Dwarfs
DOI: 10.3847/1538-3881/abe535 Bibcode: 2021AJ....161..197C

Schlaufman, Kevin C.; Chandra, Vedant

It is uncertain whether or not low-mass Population III stars ever existed. While limits on the number density of Population III stars with M* ≈ 0.8 M have been derived, using Sloan Digital Sky Survey (SDSS) data, little is known about the occurrence of Population III stars at lower masses. In the absence of reliable parallax…

2021 The Astronomical Journal
Gaia 2
Visibility analysis of Phobos to support a science and exploration platform
DOI: 10.1186/s40623-021-01542-w Bibcode: 2021EP&S...73..215S

Sefton-Nash, Elliot; Cardesín-Moinelo, Alejandro; Witasse, Olivier +3 more

The surfaces of the Martian moons, Phobos and Deimos may offer a stable environment for long-term operation of platforms. We present a broad assessment of potential scientific investigations, as well as strategic and operational opportunities offered by long-term operation of an instrumented lander. Studies using observations of Mars' moons, and t…

2021 Earth, Planets and Space
MEx 2
V488 Per Revisited: No Strong Mid-infrared Emission Features and No Evidence for Stellar/substellar Companions
DOI: 10.3847/1538-4357/ac19a8 Bibcode: 2021ApJ...922...75S

Howard, Andrew W.; Zuckerman, B.; Song, Inseok +4 more

We present characterization of the planetary system architecture for V488 Per, the dustiest main-sequence star known with a fractional infrared luminosity of ≈16%. Far-infrared imaging photometry confirms the existence of an outer planetary system dust population with a blackbody-fit temperature of ≈130 K. Mid-infrared spectroscopy probing the pre…

2021 The Astrophysical Journal
Gaia Herschel 2
Studies of emission regions of the X-ray pulsar Hercules X-1 with pulse-phase-resolved spectra observed with Suzaku
DOI: 10.1093/pasj/psaa120 Bibcode: 2021PASJ...73..286K

Dotani, Tadayasu; Inoue, Hajime; Kondo, Keisuke

Pulse-phase-resolved X-ray spectra of the X-ray pulsar Her X-1 observed with Suzaku are analyzed. The analysis is based on a hypothesis that the observed variations of the continuum spectra associated with the neutron star spin originate in the changes of the projection areas of the emission regions viewed from the observer, and that the spectral …

2021 Publications of the Astronomical Society of Japan
Suzaku 2
Broad-velocity-width Molecular Features in the Galactic Plane
DOI: 10.3847/1538-4357/abd556 Bibcode: 2021ApJ...908..246Y

Oka, Tomoharu; Tsujimoto, Shiho; Iwata, Yuhei +2 more

We performed a systematic search for broad-velocity-width molecular features (BVFs) in the disk part of our Galaxy by using the CO J = 1-0 survey data obtained with the Nobeyama Radio Observatory 45 m telescope. From this search, 58 BVFs were identified. In comparisons with the infrared and radio continuum images, 36 BVFs appeared to have both inf…

2021 The Astrophysical Journal
AKARI 2
FPGA Design for On-Board Measurement of Intermittency From In-Situ Satellite Data
DOI: 10.1029/2021EA001678 Bibcode: 2021E&SS....801678D

Echim, M. M.; Teodorescu, E.; Deak, N. +2 more

Intermittency is a fundamental property of space plasma dynamics, characterizing turbulent dynamical variables as well as passive scalars. Its qualitative and quantitative description from in-situ data requires an accurate estimation of the probability density functions (PDFs) of fluctuations and their moments, particularly the flatness, a normali…

2021 Earth and Space Science
Ulysses 2
Geological History of Southeastern Gorgonum Chaos, Mars: A Story of Water and Wind
DOI: 10.1029/2021JE006903 Bibcode: 2021JGRE..12606903H

Hauber, Ernst; Adeli, Solmaz; Haack, David

Gorgonum Chaos is part of the Eridania paleolake in Terra Sirenum and displays a number of prominent light-toned morphological features that bear a record of the regional climatic conditions throughout most of Martian history. Based on an intergrated analysis of orbital data, we mapped a 1,500 km2 area in the southeast of Gorgonum Chaos…

2021 Journal of Geophysical Research (Planets)
MEx 2