Search Publications

Properties of giant molecular clouds in the strongly barred galaxy NGC 1300
DOI: 10.1093/mnras/staa556 Bibcode: 2020MNRAS.493.5045M

Ohta, Kouji; Maeda, Fumiya; Fujimoto, Yusuke +1 more

Star formation activity depends on galactic-scale environments. To understand the variations in star formation activity, comparing the properties of giant molecular clouds (GMCs) among environments with different star formation efficiency (SFE) is necessary. We thus focus on a strongly barred galaxy to investigate the impact of the galactic enviro…

2020 Monthly Notices of the Royal Astronomical Society
eHST 17
The nature of CR7 revealed with MUSE: a young starburst powering extended Ly α emission at z = 6.6
DOI: 10.1093/mnras/staa2550 Bibcode: 2020MNRAS.498.3043M

Richard, Johan; Nanayakkara, Themiya; Sobral, David +11 more

CR7 is among the most luminous Ly α emitters (LAEs) known at z = 6.6 and consists of at least three UV components that are surrounded by Ly α emission. Previous studies have suggested that it may host an extreme ionizing source. Here, we present deep integral field spectroscopy of CR7 with VLT/Multi Unit Spectroscopic Explorer (MUSE). We measure e…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 17
A Habitable-zone Earth-sized Planet Rescued from False Positive Status
DOI: 10.3847/2041-8213/ab84e5 Bibcode: 2020ApJ...893L..27V

Vanderburg, Andrew; Bryson, Steve; Latham, David W. +9 more

We report the discovery of an Earth-sized planet in the habitable zone of a low-mass star called Kepler-1649. The planet, Kepler-1649 c, is 1.06 ${}_{-0.10}^{+0.15}$ times the size of Earth and transits its 0.1977 ± 0.0051 ${M}_{\odot }$ "mid" M-dwarf host star every 19.5 days. It receives 74% ± 3% the incident flux of Earth, giving it an equilibr…

2020 The Astrophysical Journal
Gaia 17
First detection of the carbon chain molecules 13CCC and C13CC towards SgrB2(M)
DOI: 10.1051/0004-6361/201936538 Bibcode: 2020A&A...633A.120G

Giesen, T. F.; Stutzki, J.; Simon, R. +4 more

Context. Carbon molecules and their 13C-isotopologues can be used to determine the 12C/13C abundance ratios in stellar and interstellar objects. C3 is a pure carbon chain molecule found in star-forming regions and in stellar shells of carbon-rich late-type stars. Latest laboratory data of 13C-…

2020 Astronomy and Astrophysics
Herschel 17
Magnetic Properties of Asteroid (162173) Ryugu
DOI: 10.1029/2019JE006035 Bibcode: 2020JGRE..12506035H

Motschmann, Uwe; Fujimoto, Masaki; Richter, Ingo +22 more

Observations of the magnetization state of asteroids indicate diverse properties. Values between 1.9 × 10-6 Am2/kg (Eros) and 10-2 Am2/kg (Braille) have been reported. A more detailed understanding of asteroidal magnetic properties allows far-reaching conclusions of the magnetization mechanism as well as…

2020 Journal of Geophysical Research (Planets)
Rosetta 17
NGTS clusters survey - II. White-light flares from the youngest stars in Orion
DOI: 10.1093/mnras/staa1971 Bibcode: 2020MNRAS.497..809J

Jackman, James A. G.; Wheatley, Peter J.; Moyano, Maximiliano +18 more

We present the detection of high-energy white-light flares from pre-main-sequence stars associated with the Orion Complex, observed as part of the Next Generation Transit Survey (NGTS). With energies up to 5.2 × 1035 erg these flares are some of the most energetic white-light flare events seen to date. We have used the NGTS observations…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 17
Orbital variability of the optical linear polarization of the γ-ray binary LS I +61° 303 and new constraints on the orbital parameters
DOI: 10.1051/0004-6361/202038745 Bibcode: 2020A&A...643A.170K

Piirola, Vilppu; Tsygankov, Sergey S.; Poutanen, Juri +8 more

We studied the variability of the linear polarization and brightness of the γ-ray binary LS I +61° 303. High-precision BVR photopolarimetric observations were carried out with the Dipol-2 polarimeter on the 2.2 m remotely controlled UH88 telescope at Mauna Kea Observatory and the 60 cm Tohoku telescope at Haleakala bservatory (Hawaii) over 140 nig…

2020 Astronomy and Astrophysics
Gaia 17
Estimating the Temperature and Density of a Spicule from 100 GHz Data Obtained with ALMA
DOI: 10.3847/2041-8213/ab62a5 Bibcode: 2020ApJ...888L..28S

Shibata, Kazunari; Shimojo, Masumi; Narukage, Noriyuki +6 more

We succeeded in observing two large spicules simultaneously with the Atacama Large Millimeter/submillimeter Array (ALMA), the Interface Region Imaging Spectrograph (IRIS), and the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory. One is a spicule seen in the IRIS Mg II slit-jaw images and AIA 304 Å images (Mg II/304 Å spi…

2020 The Astrophysical Journal
IRIS 17
Follow-up Studies of Five Cataclysmic Variable Candidates Discovered by LAMOST
DOI: 10.3847/1538-3881/aba7c7 Bibcode: 2020AJ....160..151T

Thorstensen, John R.

We report follow-up observations of five cataclysmic variable candidates from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) published by Hou et al. LAMOST J024048.51+195226.9 is the most unusual of the five; an early-M type secondary star contributes strongly to its spectrum, and its spectral and photometric behavior are s…

2020 The Astronomical Journal
Gaia 17
Plasma Diagnostics from Active Region and Quiet-Sun Spectra Observed by Hinode/EIS: Quantifying the Departures from a Maxwellian Distribution
DOI: 10.3847/1538-4357/ab8010 Bibcode: 2020ApJ...893...34L

Dudík, Jaroslav; Dzifčáková, Elena; Mason, Helen E. +2 more

We perform plasma diagnostics, including that of the non-Maxwellian κ-distributions, in several structures observed in the solar corona by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on board the Hinode spacecraft. To prevent uncertainties due to the in-flight calibration of EIS, we selected spectral atlases observed shortly after the launc…

2020 The Astrophysical Journal
Hinode 17