Search Publications

A new shape model of the bilobate comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2023.115566 Bibcode: 2023Icar..40115566C

Chen, Min; Huang, Xianfeng; Yan, Jianguo +2 more

In this article, we performed the stereo-photogrammetric processing on over 5200 Rosetta/OSIRIS-NAC images to derive a global high-resolution 3D model of the bilobate comet 67P/Churyumov-Gerasimenko, which is visually richer and more convincing than the existing models (i.e., SPG-SHAP4S, SPC-SHAP5 and SPG-SHAP7). This shape model was used to gener…

2023 Icarus
Rosetta 2
Active Asteroid 311P/PanSTARRS: Rotational Instability as the Origin of its Multitails?
DOI: 10.3847/1538-3881/acf31c Bibcode: 2023AJ....166..156L

Li, Fei; Liu, Bin; Liu, Xiaodong +3 more

The active asteroid 311P/PanSTARRS is one of the two targets of the planned Chinese asteroid exploration mission Tianwen-2. During 2013, 311P experienced several mass-loss events and exhibited multiple comet-like tails. Here we analyze the morphology and surface brightness of the tails to investigate the dust environment around the nucleus and the…

2023 The Astronomical Journal
eHST 2
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification
DOI: 10.3847/1538-4357/acb3a6 Bibcode: 2023ApJ...948...59C

Kargaltsev, Oleg; Chen, Steven; Yang, Hui +4 more

Open clusters are thought to be the birthplace of most stars in the galaxy. Thus, they are excellent laboratories for investigating stellar evolution, and X-ray properties of various types of stars (including binary stars, evolved stars, and compact objects). In this work, we investigate the population of X-ray sources in the nearby 300 Myr old op…

2023 The Astrophysical Journal
Gaia 2
The Bolometric Bond Albedo of Enceladus
DOI: 10.1016/j.icarus.2023.115429 Bibcode: 2023Icar..39415429L

West, Robert A.; Nixon, Conor A.; Fry, Patrick M. +13 more

The bolometric Bond albedo is a fundamental parameter of planets and moons. Here, combined observations from the Cassini spacecraft and the Hubble Space Telescope are used to determine the bolometric Bond albedo of Enceladus. We provide the full-disk reflectance of Enceladus across all phase angles (0° -180°) from 150 nm to 5131 nm, a spectral ran…

2023 Icarus
Cassini eHST 2
Infrared Galaxies Detected by the Atacama Cosmology Telescope
DOI: 10.3847/1538-4365/acb8ba Bibcode: 2023ApJS..265...45K

Kilerci, Ece; Hashimoto, Tetsuya; Goto, Tomotsugu +4 more

We report on 167 infrared (IR) galaxies selected by AKARI and IRAS and detected in the Atacama Cosmology Telescope (ACT) Data Release 5 (DR5) sky maps at the 98, 150, and 220 GHz frequency bands. Of these detections, 134 (80%) of the millimeter counterparts are first-time identifications with ACT. We expand the previous ACT extragalactic source ca…

2023 The Astrophysical Journal Supplement Series
AKARI Herschel 2
Spectral Analysis of Clay-bearing Outcrops in Northern Xanthe Terra, Mars: Comparison with Oxia Planum, the Landing Site for the ExoMars Rover Mission
DOI: 10.3847/PSJ/acb3bc Bibcode: 2023PSJ.....4...27B

Altieri, Francesca; Brossier, Jeremy; De Sanctis, Maria Cristina +5 more

Clay minerals detected on Mars are valuable targets to seek traces of life on the planet, where biosignatures might be preserved. Here, we report an in-depth spectral analysis of clay-rich outcrops identified in northern Xanthe Terra (300°-320° E, 10°-20° N). We focused particularly on the absorptions centered in the 1.0-2.6 µm spectral rang…

2023 The Planetary Science Journal
MEx 2
XMM-Newton observation of V1504 Cyg as a probe for the existence of an evaporated corona
DOI: 10.1051/0004-6361/202142725 Bibcode: 2023A&A...674A.188D

Ness, J. -U.; Dobrotka, A.; Nucita, A. A. +1 more


Aims: We present an analysis of an XMM-Newton observation of the dwarf nova V1504 Cyg during the decline from an outburst. Our goal is to search for evidence of an evaporated X-ray corona. Such a corona can be understood as an optically thin and geometrically thick disc around the central part of an optically thick and geometrically thin disc…

2023 Astronomy and Astrophysics
Gaia XMM-Newton 2
Enhanced YSO population in Serpens
DOI: 10.1007/s12036-023-09945-9 Bibcode: 2023JApA...44...41H

Saifuddin, Md.; Hasan, S. N.; Hasan, Priya +1 more

Serpens molecular cloud is one of the most active sites of ongoing star formation at a distance of about 300 pc, and hence, is very well-suited for studies of young low-mass stars and sub-stellar objects. In this paper, for the Serpens star-forming region, we found potential members of the Young Stellar Objects (YSOs) population from the Gaia DR3 …

2023 Journal of Astrophysics and Astronomy
Gaia 2
LeMMINGs. V. Nuclear activity and bulge properties: A detailed multi-component decomposition of e-MERLIN Palomar galaxies with HST
DOI: 10.1051/0004-6361/202345913 Bibcode: 2023A&A...675A.105D

Argo, M. K.; Gallagher, J. S.; Knapen, J. H. +12 more

We used high-resolution HST imaging and e-MERLIN 1.5-GHz observations of galaxy cores from the LeMMINGs survey to investigate the relation between optical structural properties and nuclear radio emission for a large sample of galaxies. We performed accurate, multi-component decompositions of new surface brightness profiles extracted from HST image…

2023 Astronomy and Astrophysics
eHST 2
Investigating Stellar Variability in the Open Cluster Region NGC 381
DOI: 10.3847/1538-3881/acad7e Bibcode: 2023AJ....165...90M

Joshi, Y. C.; Panchal, A.; Maurya, Jayanand +1 more

We study variable stars in the field of the open cluster NGC 381 using photometric data observed over 27 nights and identify a total of 57 variable stars, six of which are member stars. The variable stars are classified based on their periods, amplitudes, light-curve shapes, and locations in the H-R diagram. We found a rich variety of variable sta…

2023 The Astronomical Journal
Gaia 2