Search Publications

Firefly: A Browser-based Interactive 3D Data Visualization Tool for Millions of Data Points
DOI: 10.3847/1538-4365/acb59f Bibcode: 2023ApJS..265...38G

Geller, Aaron M.; Gurvich, Alexander B.

We present Firefly, a new browser-based interactive tool for visualizing 3D particle data sets. On a typical personal computer, Firefly can simultaneously render and enable real-time interactions with ≳10 million particles, and can interactively explore data sets with billions of particles using the included custom-built octree render engine. Once…

2023 The Astrophysical Journal Supplement Series
Gaia 1
A high-resolution spectroscopic search for multiple populations in the 2 Gyr old cluster NGC 1846
DOI: 10.1093/mnras/stac3552 Bibcode: 2023MNRAS.519..831O

Da Costa, G. S.; Mackey, A. D.; Nordlander, T. +1 more

We present detailed C, O, Na, Mg, Si, Ca, Ti, V, Fe, Zr, Ba, and Eu abundance measurements for 20 red giant branch (RGB) stars in the Large Magellanic Cloud (LMC) star cluster NGC 1846 ([Fe/H] = -0.59). This cluster is 1.95 Gyr old and lies just below the supposed lower age limit (2 Gyr) for the presence of multiple populations in massive star clu…

2023 Monthly Notices of the Royal Astronomical Society
eHST 1
A Search for Exoplanets around Northern Circumpolar Stars VII. Detection of Planetary Companion Orbiting the Largest Host Star HD 18438
DOI: 10.5303/JKAS.2023.56.1.35 Bibcode: 2023JKAS...56...35L

Lee, Byeong-Cheol; Park, Myeong-Gu; Choi, Yeon-Ho +3 more

We have been conducting a exoplanet search survey using Bohyunsen Observatory Echelle Spectrograph (BOES) for the last 18 years. We present the detection of exoplanet candidate in orbit around HD 18438 from high-precision radial velocity (RV) mesurements. The target was already reported in 2018 (Bang et al. 2018). They conclude that the RV variati…

2023 Journal of Korean Astronomical Society
Gaia Hipparcos 1
Combination of MRO SHARAD and deep-learning-based DTM to search for subsurface features in Oxia Planum, Mars
DOI: 10.1051/0004-6361/202346197 Bibcode: 2023A&A...676A..16X

Tao, Yu; Muller, Jan-Peter; Xiong, Siting +3 more

Context. Oxia Planum is a mid-latitude region on Mars that attracts a great amount of interest worldwide. An orbiting radar provides an effective way to probe the Martian subsurface and detect buried layers or geomorphological features. The Shallow radar orbital radar system on board the NASA Mars reconnaissance orbiter transmits pulsed signals to…

2023 Astronomy and Astrophysics
MEx 1
Mass Ratio Distribution of Hierarchical Triple Systems from the LAMOST-MRS Survey
DOI: 10.3847/1538-4357/acf8c4 Bibcode: 2023ApJ...958...14H

Han, Zhanwen; Chen, Xuefei; Li, Jiangdan +3 more

Hierarchical triple-star systems consists of three components organized into an inner binary (M 1, M 2) and a more distant outer tertiary (M 3) star. The LAMOST Medium-Resolution Spectroscopic Survey has offered a great sample for the study of triple-system populations. We used the peak amplitude ratio method to ob…

2023 The Astrophysical Journal
Gaia 1
Investigation into the reflection properties of the neutron star low-mass X-ray binary 4U 1636-53
DOI: 10.1051/0004-6361/202346584 Bibcode: 2023A&A...677A.156L

Wang, H. G.; García, F.; Zhang, G. B. +1 more

We present the spectroscopy of the neutron star low-mass X-ray binary 4U 1636-53 using six simultaneous XMM-Newton and Rossi X-ray Timing Explorer observations. We applied different self-consistent reflection models to explore the features when the disk is illuminated by either the corona or the neutron star surface. We found that the spectra coul…

2023 Astronomy and Astrophysics
XMM-Newton 1
RZ Piscium Hosts a Compact and Highly Perturbed Debris Disk
DOI: 10.3847/1538-4357/ad04d9 Bibcode: 2023ApJ...959...43S

Hughes, A. Meredith; Liu, Hauyu Baobab; Rieke, G. H. +6 more

RZ Piscium (RZ Psc) is well known in the variable star field because of its numerous irregular optical dips in the past 5 decades, but the nature of the system is heavily debated in the literature. We present multiyear infrared monitoring data from Spitzer and WISE to track the activities of the inner debris production, revealing stochastic infrar…

2023 The Astrophysical Journal
AKARI Gaia 1
Infrared view of the multiphase ISM in NGC 253. II. Modelling the ionised and neutral atomic gas
DOI: 10.1051/0004-6361/202347557 Bibcode: 2023A&A...680A..55B

Lebouteiller, Vianney; Ramambason, Lise; Madden, Suzanne C. +9 more

Context. Multi-wavelength studies of galaxies and galactic nuclei allow us to build a relatively more complete picture of the interstellar medium (ISM), especially in the dusty regions of starburst galaxies. An understanding of the physical processes in nearby galaxies can assist in the study of more distant sources at higher redshifts that cannot…

2023 Astronomy and Astrophysics
eHST 1
The Environment and Star Formation around the Infrared Bubble N 13
DOI: 10.1088/1674-4527/aca274 Bibcode: 2023RAA....23a5011Z

Xu, Ye; Zhou, Dong-Dong; Zhou, Jian-Jun +2 more

Infrared bubbles provide a unique opportunity to study the interactions between massive stars and surrounding material. We conduct a multi-wavelength study on the environment and star formation around an infrared bubble N 13. Three dust clumps and two molecular clumps are identified around N 13, which are all distributed on the layer. Young stella…

2023 Research in Astronomy and Astrophysics
Gaia Herschel 1
Concerning the detection of electromagnetic knot structures in space plasmas using the wave telescope technique
DOI: 10.5194/angeo-41-253-2023 Bibcode: 2023AnGeo..41..253T

Motschmann, Uwe; Glassmeier, Karl-Heinz; Toepfer, Simon

The wave telescope technique is broadly established in the analysis of spacecraft data and serves as a bridge between local measurements and the global picture of spatial structures. The technique is originally based on plane waves and has been extended to spherical waves, phase-shifted waves and planetary magnetic field representation. The goal o…

2023 Annales Geophysicae
Cluster 1