Search Publications

Organic matter in interstellar dust lost at the approach to the heliosphere. Exothermic chemical reactions of free radicals ignited by the Sun
DOI: 10.1051/0004-6361/201526964 Bibcode: 2020A&A...643A..50K

Kimura, Hiroshi; Postberg, Frank; Altobelli, Nicolas +1 more


Aims: We tackle the conundrums of organic materials missing from interstellar dust when measured inside the Solar System, while undoubtedly existing in the local interstellar cloud (LIC), which surrounds the Solar System.
Methods: We present a theoretical argument that organic compounds sublimate almost instantaneously by exothermic reac…

2020 Astronomy and Astrophysics
Ulysses 3
Ionospheric total electron content of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201937022 Bibcode: 2020A&A...635A..51H

Henri, Pierre; Hajra, Rajkumar; Galand, Marina +6 more

We study the evolution of a cometary ionosphere, using approximately two years of plasma measurements by the Mutual Impedance Probe on board the Rosetta spacecraft monitoring comet 67P/Churyumov-Gerasimenko (67P) during August 2014-September 2016. The in situ plasma density measurements are utilized to estimate the altitude-integrated electron num…

2020 Astronomy and Astrophysics
Rosetta 3
Numerical simulation and data analysis of the 23 July 2012 SEP event observed by ACE, STEREO-A, and STEREO-B
DOI: 10.1051/0004-6361/201936786 Bibcode: 2020A&A...637A..48Q

Qin, G.; Qi, S. -Y.

An extremely powerful, superfast interplanetary coronal mass ejection (ICME) from the Sun on 23 July 2012 was detected by widely separated multiple spacecraft, namely STEREO-A, STEREO-B, and ACE, together with the ICME-driven shock and associated solar energetic particles (SEPs). We use the Parker spiral magnetic field model to analyze the relatio…

2020 Astronomy and Astrophysics
SOHO 3
The Molecular Clouds Associated with the H II Regions/Candidates between L = 207°7 and L = 211°7
DOI: 10.3847/1538-4365/ab9cc0 Bibcode: 2020ApJS..249...27L

Wang, Hongchi; Ma, Yuehui; Zhang, Miaomiao +2 more

Using the PMO-13.7 m millimeter telescope at Delingha in China, we have conducted a large-scale simultaneous survey of 12CO, 13CO, and C18O J = 1 - 0 emission toward the sky region centered at l = 209°7, b = -2°25 with a coverage of 4°0 × 4°5. The majority of the emission in the region comes from the clouds with ve…

2020 The Astrophysical Journal Supplement Series
Gaia 3
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