Search Publications

Extensive Secondary Cratering From the InSight Sol 1034a Impact Event
DOI: 10.1029/2024JE008535 Bibcode: 2024JGRE..12908535G

Grindrod, P. M.; Daubar, I. J.; Collins, G. S. +10 more

Impact cratering is one of the fundamental processes throughout the history of the Solar System. The formation of new impact craters on planetary bodies has been observed with repeat images from orbiting satellites. However, the time gap between images is often large enough to preclude detailed analysis of smaller-scale features such as secondary …

2024 Journal of Geophysical Research (Planets)
MEx 0
Some observational properties of the Herbig Be Star AS 310
DOI: 10.1016/j.asr.2023.12.052 Bibcode: 2024AdSpR..73.3300I

Bakış, Volkan; Alishov, S. A.; Ismailov, Nariman Z. +2 more

The results of spectral and photometric studies of Herbig Be-type star AS 310 have been presented. Photometric observations in the BVRcIc bands performed in 2016-2021 showed that the amplitude of the seasonal brightness variations of the star changes smoothly in different years and reaches a maximum of approximately around Δ V ∼ 0.6 mag in 2018. T…

2024 Advances in Space Research
Gaia 0
An Inward-moving and Asymmetric Velocity Wave Detected in LAMOST-Gaia
DOI: 10.3847/2041-8213/ad18a7 Bibcode: 2024ApJ...961L...4C

Zhao, Gang; Chen, Yuqin; Wu, Wenbo +3 more

The phase space, as coded by kinematic parameters and chemical abundances, is crucial for understanding the formation of the Galactic disk. Using red giant stars from the Galactic thin disk with [Fe/H] > - 0.8 and low-α ratios identified in LAMOST-Gaia, we detect numerous ridges and undulations in the R-V ϕ diagram coded by median …

2024 The Astrophysical Journal
Gaia 0
NGC 2403 XMM4: evidence for a super-Eddington neutron star with a possible transient pulsation
DOI: 10.1093/mnras/stae023 Bibcode: 2024MNRAS.528..418L

Roberts, Timothy P.; Luangtip, Wasutep

We present a study of the X-ray source NGC 2403 XMM4 (4XMM J073702.2+653934) based on 20 yr of archival observations with XMM-Newton, Chandra, Swift, and NuSTAR. Although it has previously been classified as an ultraluminous X-ray source (ULX), we show that its luminosity rarely, if ever, passes the $10^{39} \rm \, erg \, s^{-1}$ threshold luminos…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Deuterium fractionation in cold dense cores in the low-mass star-forming region L1688
DOI: 10.1093/mnras/stae116 Bibcode: 2024MNRAS.528.1327P

Caselli, P.; Pineda, J. E.; Sipilä, O. +5 more

In this work, we study deuterium fractionation in four starless cores in the low-mass star-forming region L1688 in the Ophiuchus molecular cloud. We study how the deuterium fraction (RD) changes with environment, compare deuteration of ions and neutrals, core centre and its envelope, and attempt to reproduce the observed results with a …

2024 Monthly Notices of the Royal Astronomical Society
Herschel 0
Complex dayside particle precipitation observed during the passage of a solar wind rotational discontinuity
DOI: 10.3389/fspas.2024.1320809 Bibcode: 2024FrASS..1120809W

Escoubet, C. Philippe; Wing, Simon; Berchem, Jean +1 more

The dayside particle precipitation during the passage of a solar wind rotational discontinuity (RD) event on 10 April 2015 is examined and reviewed. The RD leads to complex structures at the magnetopause, boundary layer, mantle, and cusp even though the geomagnetic activity level remains low. Particle precipitation data from DMSP F17 reveal the fo…

2024 Frontiers in Astronomy and Space Sciences
Cluster 0
The nature of very-faint X-ray binaries: near-infrared spectroscopy of 1RXH J173523.7-354013 reveals a giant companion
DOI: 10.1093/mnras/stad3693 Bibcode: 2024MNRAS.527.7603S

Maccarone, T. J.; Degenaar, N.; Wijnands, R. +3 more

Very-faint X-ray binaries (VFXBs) are a subclass of black holes and neutron stars in binaries that appear to be accreting at a very low rate. In addition to providing interesting constraints on poorly understood forms of accretion, elucidating the nature of VFXBs is particularly interesting for binary evolution and population modelling. Through ne…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0
A Multiwavelength Portrait of the 3C 220.3 Lensed System
DOI: 10.3847/1538-4357/ad68f7 Bibcode: 2024ApJ...974..171H

Azadi, Mojegan; Wilkes, Belinda J.; Worrall, D. M. +10 more

The 3C 220.3 system is a rare case of a foreground narrow-line radio galaxy ("galaxy A," z A = 0.6850) lensing a background submillimeter galaxy (z SMG = 2.221). New spectra from MMT/Binospec confirm that the companion galaxy ("galaxy B") is part of the lensing system with z B = 0.6835. New three-color Hubble S…

2024 The Astrophysical Journal
Herschel eHST 0
G213.0-0.6, a true supernova remnant or just an H II region?
DOI: 10.1093/mnras/stad3596 Bibcode: 2024MNRAS.527.7355G

Han, J. L.; Reich, W.; Gao, X. Y. +2 more

G213.0-0.6 is a faint extended source situated in the anticentre region of the Galactic plane. It has been classified as a shell-type supernova remnant (SNR) based on its shell-like morphology, steep radio continuum spectrum, and high ratio of [S II]/Hα. With new optical emission line data of Hα, [S II], and [N II] recently observed by the Large S…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0
From SMART1 and recent probes towards Artemis and a human/robotic Moon Village
DOI: 10.1088/1742-6596/2877/1/012037 Bibcode: 2024JPhCS2877a2037F

Foing, Bernard

This paper describes highlights of some of the European Space Agency (ESA) missions to the Moon, such as the 2003 ESA SMART-1 Mission to the Moon and the fleet of orbital missions from 2007 that changed our views of the Moon. It discusses the International Lunar Exploration Working Group (ILEWG) MoonVillage roadmap towards a series of landers or a…

2024 Journal of Physics Conference Series
SMART-1 0