Search Publications

Discovery of the Longest-period Classical Cepheid in the Milky Way
DOI: 10.3847/2041-8213/ad392f Bibcode: 2024ApJ...965L..17S

Soszyński, I.; Udalski, A.; Szymański, M. K. +12 more

We report the discovery of the classical Cepheid OGLE-GD-CEP-1884 (= GDS_J1535467-555656) with the longest pulsation period known in our Galaxy. The period of 78.14 days is nearly 10 days longer than that of the previous record-holding Cepheid, S Vulpeculae, and thus, OGLE-GD-CEP-1884 can be categorized as the first ultra-long-period Cepheid in th…

2024 The Astrophysical Journal
Gaia 4
Magnetic Fields in M-dwarf Members of the Pleiades Open Cluster Using APOGEE Spectra
DOI: 10.3847/1538-4357/ad571f Bibcode: 2024ApJ...971..112W

Wanderley, Fábio; Cunha, Katia; Smith, Verne V. +10 more

Average magnetic field measurements are presented for 62 M-dwarf members of the Pleiades open cluster, derived from Zeeman-enhanced Fe I lines in the H band. A Markov Chain Monte Carlo methodology was employed to model magnetic filling factors using Sloan Digital Sky Survey (SDSS) IV APOGEE high-resolution spectra, along with the radiative transfe…

2024 The Astrophysical Journal
Gaia 4
Dark Photon Dark Matter and Low-frequency Gravitational-wave Detection with Gaia-like Astrometry
DOI: 10.3847/1538-4357/ad89b9 Bibcode: 2024ApJ...976..247A

Wang, Xin; Zhao, Yue; An, Haipeng +3 more

Astrometric surveys offer us a method for searching for elusive cosmic signatures, such as ultralight dark photon dark matter and gravitational waves (GWs), by observing the temporal change of stars' apparent locations. The detection capabilities of such surveys rapidly decrease at low frequencies, because the signals become hardly distinguishable…

2024 The Astrophysical Journal
Gaia 4
Blowing Star Formation Away in Active Galactic Nuclei Hosts. I. Observation of Warm Molecular Outflows with JWST MIRI
DOI: 10.3847/1538-4357/ad702a Bibcode: 2024ApJ...974..127C

Riffel, Rogério; Zakamska, Nadia L.; Storchi-Bergmann, Thaisa +4 more

We use the James Webb Space Telescope Mid-Infrared Instrument medium-resolution spectrometer observations of the radio-loud active galactic nucleus (AGN) host UGC 8782 to map the warm molecular and ionized gas kinematics. The data reveal spatially resolved outflows in the inner 2 kpc, seen in low ionization (traced by the [Ar II] 6.99 µm emi…

2024 The Astrophysical Journal
JWST 4
Observation of a Fully-formed Forward–Reverse Shock Pair due to the Interaction between Two Coronal Mass Ejections at 0.5 au
DOI: 10.3847/2041-8213/ad68fa Bibcode: 2024ApJ...971L..35T

Lugaz, Noé; Wimmer-Schweingruber, Robert F.; Dresing, Nina +17 more

We report direct observations of a fast magnetosonic forward–reverse shock pair observed by Solar Orbiter on 2022 March 8 at the short heliocentric distance of 0.5 au. The structure, sharing some features with fully-formed stream interaction regions, is due to the interaction between two successive coronal mass ejections (CMEs), never previously o…

2024 The Astrophysical Journal
SOHO SolarOrbiter 4
The First Combined Hα and Rest-UV Spectroscopic Probe of Galactic Outflows at High Redshift
DOI: 10.3847/1538-4357/ad7ebb Bibcode: 2024ApJ...976...28K

Tacconi, L. J.; Shapley, Alice E.; Reddy, Naveen A. +6 more

We investigate the multiphase structure of gas flows in galaxies. We study 80 galaxies during the epoch of peak star formation (1.4 ≤ z ≤ 2.7) using data from the Keck/Low-Resolution Imaging Spectrometer (LRIS) and the Very Large Telescope/K-Band Multi-Object Spectrograph (KMOS). Our analysis provides a simultaneous probe of outflows using UV emis…

2024 The Astrophysical Journal
Herschel 4
Evidence of Continuous Reconnection along a Helmet Streamer Current Sheet Observed by WISPR on Parker Solar Probe
DOI: 10.3847/1538-4357/ad509b Bibcode: 2024ApJ...970...79L

Vourlidas, Angelos; Qiu, Jiong; Stenborg, Guillermo +5 more

Parker Solar Probe's second solar encounter from 2019 March 30 to April 11 occurred during a period when the corona had a simple magnetic structure and relatively flat heliospheric current sheet (HCS), which was in the field of view of the Wide-field Imager for Solar Probe (WISPR) throughout. The images show an almost continual flow of transient d…

2024 The Astrophysical Journal
SOHO 4
The Truncated Circumgalactic Medium of the Large Magellanic Cloud
DOI: 10.3847/2041-8213/ad8b9d Bibcode: 2024ApJ...976L..28M

Fox, Andrew J.; Lehner, Nicolas; Tumlinson, Jason +6 more

The Large Magellanic Cloud (LMC) is the nearest massive galaxy to the Milky Way (MW). Its circumgalactic medium (CGM) is complex and multiphase, containing both stripped H I structures like the Magellanic Stream and Bridge and a diffuse warm corona seen in high-ion absorption. We analyze 28 active galactic nucleus sight lines passing within 35 kpc…

2024 The Astrophysical Journal
eHST 4
Active Galactic Nucleus Properties of ∼1 Million Member Galaxies of Galaxy Groups and Clusters at z < 1.4 Based on the Subaru Hyper Suprime-Cam Survey
DOI: 10.3847/1538-4357/ad32c6 Bibcode: 2024ApJ...967...65T

Goto, Tomotsugu; Imanishi, Masatoshi; Schramm, Malte +17 more

Herein, we present the statistical properties of active galactic nuclei (AGNs) for approximately 1 million member galaxies of galaxy groups and clusters with 0.1 < cluster redshift (z cl) < 1.4 selected using the Subaru Hyper Suprime-Cam, the so-called CAMIRA clusters. In this research, we focused on the AGN power fraction (f

2024 The Astrophysical Journal
eHST 4
On the Properties of X-Ray Corona in Seyfert 1 Galaxies
DOI: 10.3847/1538-4357/ad8088 Bibcode: 2024ApJ...976..145P

Stalin, C. S.; Ricci, Claudio; Marchesi, S. +4 more

We carried out a uniform and systematic analysis of a sample of 112 nearby bright Seyfert 1 type active galactic nuclei, the observations of which were carried out by the Nuclear Spectroscopic Telescope Array between 2013 August and 2022 May. The main goal of this analysis is to investigate the nature of the X-ray corona in Seyfert 1 galaxies. By …

2024 The Astrophysical Journal
INTEGRAL 4