Search Publications

Herschel Investigation of Cores and Filamentary Structures in the Perseus Molecular Cloud
DOI: 10.1088/1674-4527/ac5bc7 Bibcode: 2022RAA....22e5012Z

Zhang, Guo-Yin; Zhang, Chang; Li, Jin-Zeng +1 more

Cores and filamentary structures are the prime birthplaces of stars, and play key roles in the process of star formation. Latest advances in the methods of multi-scale source and filament extraction, and in making high-resolution column density map from Herschel multi-wavelength observations enable us to detect the filamentary network structures i…

2022 Research in Astronomy and Astrophysics
Herschel 5
An Efficient High-Resolution Global-Local Network to Detect Lunar Features for Space Energy Discovery
DOI: 10.3390/rs14061391 Bibcode: 2022RemS...14.1391J

Liu, Lei; Jia, Yutong; Peng, Siqing +2 more

Lunar craters and rilles are significant topographic features on the lunar surface that will play an essential role in future research on space energy resources and geological evolution. However, previous studies have shown low efficiency in detecting lunar impact craters and poor accuracy in detecting lunar rilles. There is no complete automated …

2022 Remote Sensing
MEx 5
Direct Evidence of Magnetic Reconnection Onset via the Tearing Instability
DOI: 10.3389/fspas.2022.869491 Bibcode: 2022FrASS...9.9491B

Verscharen, Daniel; Walsh, Andrew P.; Forsyth, Colin +4 more

Magnetic reconnection is a sporadic process responsible for energy release in space and laboratory plasmas. It is believed that the tearing mode instability may be responsible for the onset of reconnection in the magnetotail. However, due to its elusive nature, there is an absence of in-situ observations of the tearing instability prior to magneti…

2022 Frontiers in Astronomy and Space Sciences
Cluster 5
The ALPINE-ALMA [C II] Survey: The Infrared-Radio Correlation and Active Galactic Nucleus Fraction of Star-forming Galaxies at z 4.4-5.9
DOI: 10.3847/1538-4357/ac81c5 Bibcode: 2022ApJ...935..177S

Shen, Lu; Koekemoer, Anton M.; Jones, Gareth C. +26 more

We present the radio properties of 66 spectroscopically confirmed normal star-forming galaxies (SFGs) at 4.4 < z < 5.9 in the COSMOS field that were [C II]-detected in the Atacama Large Millimeter/submillimeter Array Large Program to INvestigate [C II] at Early times (ALPINE). We separate these galaxies ("C II-detected-all") into lower-redsh…

2022 The Astrophysical Journal
eHST 5
Pre- and Post-entry, Descent and Landing Assessment of the Martian Atmosphere for the Mars 2020 Rover
DOI: 10.3847/PSJ/ac7148 Bibcode: 2022PSJ.....3..147M

Kleinböhl, Armin; Mischna, Michael A.; Lewis, Stephen R. +10 more

This review provides an analysis of activities undertaken by the Mars 2020 Council of Atmospheres (CoA) in support of the entry, descent, and landing (EDL) of the Mars 2020 rover Perseverance in Jezero crater, Mars. The activities of the CoA were designed to evaluate the safety of early-stage landing site candidates and, later, to constrain the ra…

2022 The Planetary Science Journal
MEx 5
The Mars Oxygen Visible Dayglow: A Martian Year of NOMAD/UVIS Observations
DOI: 10.1029/2022JE007220 Bibcode: 2022JGRE..12707220S

Aoki, S.; Vandaele, A. C.; Daerden, F. +12 more

The Ultraviolet and Visible Spectrometer Ultraviolet (UVIS UV) and Visible Spectrometer channel of the Nadir and Occultation for MArs Discovery spectrometer aboard the ExoMars Trace Gas Orbiter has made limb observations of the Martian dayglow during more than a Martian year. Two pointing modes have been applied: (a) In the inertial mode, the spec…

2022 Journal of Geophysical Research (Planets)
ExoMars-16 5
Discovery of a pulse-phase-transient cyclotron line in the X-ray pulsar Swift J1808.4-1754 and identification of an optical companion
DOI: 10.1093/mnras/stac1462 Bibcode: 2022MNRAS.514.2707S

Tsygankov, Sergey S.; Lutovinov, Alexander A.; Molkov, Sergey V. +3 more

In this work, the temporal and spectral properties of the poorly studied X-ray pulsar Swift J1808.4-1754 were investigated in the 0.8-79 keV energy range based on the data from the NuSTAR and Swift observatories collected during the 2014 outburst. Strong pulsations with a period of 909.73 ± 0.03 s were detected in the source light curve, with the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
Spectroscopic Study of Four Metal-poor Carbon Stars from the Hamburg/ESO Survey: On Confirming the Low-mass Nature of Their Companions
DOI: 10.3847/1538-4357/ac7aac Bibcode: 2022ApJ...934..110S

Shejeelammal, J.; Goswami, Aruna

Elemental abundances of extrinsic carbon stars provide insight into the poorly understood origin and evolution of elements in the early Galaxy. In this work, we present the results of a detailed spectroscopic analysis of four potential carbon star candidates from the Hamburg/ESO Survey (HES): HE 0457-1805, HE 0920-0506, HE 1241-0337, and HE 1327-2…

2022 The Astrophysical Journal
Gaia 5
Predicting HCN, HCO+, multi-transition CO, and dust emission of star-forming galaxies. Constraining the properties of resolved gas and dust disks of local spiral galaxies
DOI: 10.1051/0004-6361/202142480 Bibcode: 2022A&A...663A.152L

Braine, J.; Bigiel, F.; Gratier, P. +2 more

The interstellar medium is a turbulent, multiphase, and multi-scale medium that follows scaling relations that link the surface density, volume density, and velocity dispersion with the cloud size. Galactic clouds range from below 1 pc to about 100 pc in size. Extragalactic clouds appear to follow the same range, although they are only now becomin…

2022 Astronomy and Astrophysics
Herschel 5
An Integrative Analysis of the Rich Planetary System of the Nearby Star e Eridani: Ideal Targets for Exoplanet Imaging and Biosignature Searches
DOI: 10.3847/1538-3881/ac6f58 Bibcode: 2022AJ....164...12B

Apai, Dániel; Dietrich, Jamie; Basant, Ritvik

e Eridani, the fifth-closest Sun-like star, hosts at least three planets and could possibly harbor more. However, the veracity of the planet candidates in the system and its full planetary architecture remain unknown. Here we analyze the planetary architecture of e Eridani via DYNAMITE, a method providing an integrative assessment of the system ar…

2022 The Astronomical Journal
Gaia 5