Search Publications

The miniJPAS survey: stellar atmospheric parameters from 56 optical filters
DOI: 10.1093/mnras/stac3155 Bibcode: 2023MNRAS.518.2018Y

Yuan, H. -B.; Solano, E.; Mendes de Oliveira, C. +29 more

With a unique set of 54 overlapping narrow-band and two broader filters covering the entire optical range, the incoming Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will provide a great opportunity for stellar physics and near-field cosmology. In this work, we use the miniJPAS data in 56 J-PAS filters and 4 compleme…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Photometric variability of blue straggler stars in M67 with TESS and K2
DOI: 10.1093/mnras/stad1947 Bibcode: 2023MNRAS.524.1360V

Bowman, Dominic M.; Jadhav, Vikrant V.; Subramaniam, Annapurni +1 more

Blue straggler stars (BSSs) are formed through mass transfers or mergers in binaries. The recent detections of white dwarf (WD) companions to BSSs in M67 suggested a mass transfer pathway of formation. In search of a close companion to five BSSs in M67 that are known to be spectroscopic binaries, we study the light curves from K2 and TESS data. We…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Radio continuum and OH line emission of high-z OH megamaser galaxies
DOI: 10.1051/0004-6361/202245347 Bibcode: 2023A&A...669A.148W

Zhu, Ming; Jiang, Peng; Zhang, Bo +8 more

We present a study of the arcsecond-scale radio continuum and OH line emission of a sample of known OH megamaser (OHM) galaxies with z ≥ 0.15 using archival Very Large Array (VLA) data and also the results of our pilot Five-hundred-meter Aperture Spherical radio Telescope (FAST) observations of 12 of these OHM galaxies. The arcsecond-scale resolut…

2023 Astronomy and Astrophysics
eHST 3
On the influence of shock-cloud interactions on the nonthermal X-ray emission from the supernova remnant RCW 86
DOI: 10.1093/pasj/psad075 Bibcode: 2023PASJ...75.1344B

Vink, Jacco; Bamba, Aya; Sano, Hidetoshi +1 more

The effect of the surrounding environment of supernova remnant shocks on nonthermal X-rays from accelerated electrons, with or without interacting dense material, is an open issue. We conduct spatially resolved X-ray spectroscopy of the shock-cloud interacting region of RCW 86 with XMM-Newton. It is found that bright soft X-ray filaments surround …

2023 Publications of the Astronomical Society of Japan
XMM-Newton 3
Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N
DOI: 10.3847/1538-4365/acbcbe Bibcode: 2023ApJS..265...50C

Bizyaev, Dmitry; Schneider, Donald P.; Mahadevan, Suvrath +12 more

We report the characterization of 28 low-mass (0.02 M ≤ M 2 ≤ 0.25 M ) companions to Kepler objects of interest (KOIs), eight of which were previously designated confirmed planets. These objects were detected as transiting companions to Sunlike stars (G and F dwarfs) by the Kepler mission and are confirmed as si…

2023 The Astrophysical Journal Supplement Series
Gaia 3
Comparison of the Composition of ICMEs from Active Regions and Quiet-Sun Regions
DOI: 10.3847/1538-4357/acba90 Bibcode: 2023ApJ...945..163L

Chen, Yao; Fu, Hui; Li, Leping +4 more

The composition of interplanetary coronal mass ejections (ICMEs), including the ionic charge states and elemental abundances of heavy elements, is tightly correlated with their source regions and eruption processes. This can help in analyzing the eruption mechanisms and plasma origins of CMEs, and deepen our understanding of energetic solar activi…

2023 The Astrophysical Journal
SOHO 3
Globular Clusters in NGC 4839 Falling into Coma: Evidence for the Second Infall?
DOI: 10.3847/1538-4357/acb1b1 Bibcode: 2023ApJ...944...51O

Lee, Myung Gyoon; Jang, In Sung; Oh, Seong-A.

NGC 4839 is the brightest galaxy (cD) of the NGC 4839 group at R ≈ 1 Mpc in the southwest of the Coma cluster, which is known to be falling into Coma. However, it has been controversial whether it is in the first phase of infall or in the second phase of infall after passing the Coma center. We present a wide field study of globular clusters (GCs)…

2023 The Astrophysical Journal
XMM-Newton 3
Made-to-measure modelling of globular clusters
DOI: 10.1093/mnras/stad762 Bibcode: 2023MNRAS.521.3898W

Bovy, Jo; Hunt, Jason A. S.; Webb, Jeremy J.

We present the first application of the made-to-measure method for modelling dynamical systems to globular clusters. Through the made-to-measure algorithm, the masses of individual particles within a model cluster are adjusted while the system evolves forward in time via a gravitational N-body code until the model cluster is able to reproduce sele…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Kepler Bonus: Light Curves of Kepler Background Sources
DOI: 10.3847/1538-3881/ad0727 Bibcode: 2023AJ....166..265M

Hedges, Christina; Martínez-Palomera, Jorge; Dotson, Jessie

NASA's Kepler primary mission observed about 116 deg2 in the sky for 3.5 consecutive years to discover Earth-like exoplanets. This mission recorded pixel cutouts, known as target pixel files (TPFs), of over 200,000 targets that were selected to maximize the scientific yield. The Kepler pipeline performed aperture photometry for these pr…

2023 The Astronomical Journal
Gaia 3
A Statistical Relation between Mass, Age, and Velocity Dispersion in the Solar Neighborhood
DOI: 10.3847/1538-4357/acb548 Bibcode: 2023ApJ...945...75F

Sajadian, Sedighe; Fatheddin, Hossein

The stellar kinematics of the Galactic disk are the main factors constraining disk formation and evolution processes in the Milky Way. In this paper, we investigate a statistical relation between stellar mass, age, and velocity dispersion for stars in the solar neighborhood. Age-velocity dispersion relations, with their applications, have been stu…

2023 The Astrophysical Journal
Gaia 3