Search Publications

Modeling ALMA Observations of the Warped Molecular Gas Disk in the Red Nugget Relic Galaxy NGC 384
DOI: 10.3847/1538-4357/ad7bb0 Bibcode: 2024ApJ...975..179C

Ho, Luis C.; Gebhardt, Karl; Barth, Aaron J. +9 more

We present 0.″22 resolution CO(2–1) observations of the circumnuclear gas disk in the local compact galaxy NGC 384 with the Atacama Large Millimeter/submillimeter Array (ALMA). While the majority of the disk displays regular rotation with projected velocities rising to 370 km s‑1, the inner ∼0.″5 exhibits a kinematic twist. We develop w…

2024 The Astrophysical Journal
eHST 4
Probing the magnetic field and dust grain properties of two dark clouds L1495 and L1498 through photopolarimetry
DOI: 10.1093/mnras/stae412 Bibcode: 2024MNRAS.528.7156C

Pandey, J. C.; Medhi, B. J.; Das, H. S. +2 more

We present the R-band polarimetry of two low-latitude Lynd's clouds L1495 and L1498 acquired with AIMPOL at Aryabhatta Research Institute of Observational Sciences, Nainital, India. The estimated polarization across the regions of L1495 and L1498 is typically in the range of ~1-5 per cent and the position angle is typically in the range of ~100°-1…

2024 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 4
Intermediate-mass black holes in Green pea galaxies (IMBH-GP) I: A candidate sample from LAMOST and SDSS
DOI: 10.1007/s11433-024-2412-3 Bibcode: 2024SCPMA..6709811L

Jiang, Linhua; Zheng, Zhen-Ya; Wang, Jun-Xian +8 more

The scaling relation of central massive black holes (MBHs) and their host galaxies is well-studied for supermassive BHs (SMBHs, MBH ≥ 106M). However, this relation has large uncertainties in the mass range of the intermediate-mass BHs (IMBHs, MBH ∼ 103–106M). Since Gree…

2024 Science China Physics, Mechanics, and Astronomy
XMM-Newton 4
Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets
DOI: 10.3847/1538-4365/ad18c3 Bibcode: 2024ApJS..271...16D

Mayo, Andrew W.; Rice, Malena; Kane, Stephen R. +29 more

Discovering and characterizing exoplanets at the outer edge of the transit method's sensitivity has proven challenging owing to geometric biases and the practical difficulties associated with acquiring long observational baselines. Nonetheless, a sample of giant exoplanets on orbits longer than 100 days has been identified by transit hunting missi…

2024 The Astrophysical Journal Supplement Series
Gaia 4
Comparison of the On-disk Apparent Current Sheets with the Limb Ones
DOI: 10.3847/1538-4357/ad6df5 Bibcode: 2024ApJ...974..104D

Zhang, Jun; Ding, Tao

Based on observations from the Solar Dynamics Observatory (SDO) and the Solar and Heliospheric Observatory (SOHO), we investigate 30 apparent current sheets during 1999–2021, including 10 on-disk and 8 limb ones from the SDO, as well as 12 limb ones from the SOHO. Each on-disk current sheet is formed among an X-type configuration consisting of two…

2024 The Astrophysical Journal
SOHO 4
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert
DOI: 10.1093/mnras/stae1420 Bibcode: 2024MNRAS.532.1612H

Butler, R. Paul; Bieryla, Allyson; Fernández Fernández, Jorge +40 more

We report the discovery of two transiting planets detected by the Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V and an F8V star, respectively, with periods of 4.31 and 1.27 d, respectively. We confirm and characterize these two planets with a variety of ground-based and follow-up observations, including ph…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 4
Firmamento: A Multimessenger Astronomy Tool for Citizen and Professional Scientists
DOI: 10.3847/1538-3881/ad216a Bibcode: 2024AJ....167..116T

Giommi, Paolo; Doro, Michele; Pollock, A. M. T. +12 more

Firmamento (https://firmamento.hosting.nyu.edu) is a new-concept, web-based, and mobile-friendly data analysis tool dedicated to multifrequency/multimessenger emitters, as exemplified by blazars. Although initially intended to support a citizen researcher project at New York University–Abu Dhabi, Firmamento has evolved to be a valuable tool for pr…

2024 The Astronomical Journal
XMM-Newton 4
Identifying synergies between VLBI and STIX imaging
DOI: 10.1051/0004-6361/202348040 Bibcode: 2024A&A...684A..47M

Massa, Paolo; Müller, Hendrik; Mus, Alejandro +2 more

Context. Reconstructing an image from noisy, sparsely sampled Fourier data is an ill-posed inverse problem that occurs in a variety of subjects within science, including data analysis for Very Long Baseline Interferometry (VLBI) and the Spectrometer/Telescope for Imaging X-rays (STIX) with respect to solar observations. The need for high-resolutio…

2024 Astronomy and Astrophysics
SolarOrbiter 4
The 3D Kinematics of the Orion Nebula Cluster. II. Mass-dependent Kinematics of the Inner Cluster
DOI: 10.3847/1538-4357/ad1401 Bibcode: 2024ApJ...962..174W

Lu, Jessica R.; Kim, Dongwon; Hsu, Chih-Chun +3 more

We present the kinematic analysis of 246 stars within $4^{\prime} $ from the center of Orion Nebula Cluster (ONC), the closest massive star cluster with active star formation across the full mass range, which provides valuable insights in the formation and evolution of star cluster on an individual-star basis. High-precision radial velocities and …

2024 The Astrophysical Journal
Gaia eHST 4
Characteristics and energy flux distributions of decayless transverse oscillations depending on coronal regions
DOI: 10.1051/0004-6361/202450433 Bibcode: 2024A&A...689A..16L

Van Doorsselaere, Tom; Lim, Daye; Berghmans, David +1 more

Context. It has been proposed that the slope (δ) of the power-law distribution between the energy flux and oscillation frequency could determine whether high-frequency transverse oscillations make a dominant contribution to the heating (δ < 1). A meta-analysis of decayless transverse oscillations revealed that high-frequency oscillations potent…

2024 Astronomy and Astrophysics
SolarOrbiter 4