Search Publications

Self-similar Buildup and Inside-out Growth: Tracing the Evolution of Intermediate-to-high-mass Star-forming Galaxies since z = 2
DOI: 10.3847/1538-4357/ad807f Bibcode: 2024ApJ...975..252H

Tacchella, Sandro; Mosleh, Moein; Hosseini-ShahiSavandi, S. Zahra +1 more

We aim to discern scenarios of structural evolution of intermediate-to-high-mass star-forming galaxies (SFGs) since cosmic noon by comparing their stellar mass profiles with present-day stellar masses of log(M

2024 The Astrophysical Journal
eHST 3
The Age-dependent Vertical Actions of Young Stars in the Galaxy
DOI: 10.3847/1538-4357/ad61e8 Bibcode: 2024ApJ...972..155G

Xiang, Maosheng; Rix, Hans-Walter; Zari, Eleonora +2 more

Stars in the Galactic disk are born on cold, nearly circular orbits with small vertical excursions. After their birth, their orbits evolve, driven by small- or large-scale perturbations in the Galactic disk's gravitational potential. Here, we study the vertical motions of young stars over their first few orbital periods, using a sample of OBA star…

2024 The Astrophysical Journal
Gaia 3
The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc
DOI: 10.3847/1538-3881/ad267d Bibcode: 2024AJ....167..174C

Skiff, Brian A.; Hartman, Zachary D.; Ciardi, David R. +8 more

M dwarfs are ubiquitous in our Galaxy, and the rate at which they host stellar companions, and the properties of these companions, provide a window into the formation and evolution of the star(s), and of any planets that they may host. The Pervasive Overview of "Kompanions" of Every M dwarf in Our Neighborhood (POKEMON) speckle survey of nearby M …

2024 The Astronomical Journal
Gaia 3
The Molecular Exoskeleton of the Ring-like Planetary Nebula NGC 3132
DOI: 10.3847/1538-4357/ad2848 Bibcode: 2024ApJ...965...21K

Wilner, David J.; De Marco, Orsola; Kastner, Joel H. +4 more

We present Submillimeter Array (SMA) mapping of 12CO J = 2 → 1, 13CO J = 2 → 1, and CN N = 2 → 1 emission from the ring-like planetary nebula NGC 3132, one of the subjects of JWST Early Release Observation near-infrared imaging. The ∼5″ resolution SMA data demonstrate that the Southern Ring's main, bright, molecule-rich ring …

2024 The Astrophysical Journal
JWST 3
Binary neutron star merger offsets from their host galaxies: GW 170817 as a case study
DOI: 10.1051/0004-6361/202450908 Bibcode: 2024A&A...692A..21G

Lyman, J. D.; Levan, A. J.; Chrimes, A. A. +2 more

Aims. The locations of binary neutron star (BNS) mergers within their host galaxies encode the systemic kicks that these systems received in the supernova aftermath. We investigate how the galactic potential and the systemic kicks shape the offset distribution of BNS mergers with a case study of GW 170817 and its host NGC 4993. Methods. We derived…

2024 Astronomy and Astrophysics
eHST 3
The ZTF Source Classification Project. III. A Catalog of Variable Sources
DOI: 10.3847/1538-4365/ad33c6 Bibcode: 2024ApJS..272...14H

Riddle, Reed; Szkody, Paula; Graham, Matthew J. +22 more

The classification of variable objects provides insight into a wide variety of astrophysics ranging from stellar interiors to galactic nuclei. The Zwicky Transient Facility (ZTF) provides time-series observations that record the variability of more than a billion sources. The scale of these data necessitates automated approaches to make a thorough…

2024 The Astrophysical Journal Supplement Series
Gaia 3
Multiwavelength Spectral Energy Distribution Analysis of X-Ray Selected Active Galactic Nuclei at z = 0.2–0.8 in the Stripe 82 Region
DOI: 10.3847/1538-4357/ad1186 Bibcode: 2024ApJ...961..246S

Ueda, Yoshihiro; Toba, Yoshiki; Li, Junyao +3 more

We perform a systematic, multiwavelength spectral energy distribution (SED) analysis of X-ray detected active galactic nuclei (AGNs) at z = 0.2–0.8 with Sloan Digital Sky Survey (SDSS) counterparts in the Stripe 82 region, consisting of 60 type 1 and 137 type 2 AGNs covering a 2–10 keV luminosity range of $41.6\lt \mathrm{log}\ {L}_{{\rm{x}}}\lt 4…

2024 The Astrophysical Journal
Herschel XMM-Newton 3
Fractionation in young cores: Direct determinations of nitrogen and carbon fractionation in HCN
DOI: 10.1051/0004-6361/202449344 Bibcode: 2024A&A...685A.149J

Caselli, P.; Jensen, S. S.; Spezzano, S. +4 more

Context. Nitrogen fractionation is a powerful tracer of the chemical evolution during star and planet formation. It requires robust determinations of the nitrogen fractionation across different evolutionary stages.
Aims: We aim to determine the 14N/15N and 12C/13C ratios for HCN in six starless and …

2024 Astronomy and Astrophysics
Herschel 3
Updated Kinematics of the Radcliffe Wave: Nonsynchronous, Dipole-like Vertical Oscillations
DOI: 10.3847/1538-4357/ad66cd Bibcode: 2024ApJ...971..167Z

Fang, Min; Li, Guang-Xing; Wang, Junzhi +6 more

The kinematic information of the Radcliffe wave (RW) is essential for determining its existence and gaining insights into its origin and evolution. In this work, we present an accurate measurement of the vertical velocity (V Z ) of the RW by incorporating the radial velocity (RV) measures through two methods, which is crucial but was n…

2024 The Astrophysical Journal
Gaia 3
NIR spectral classification of the companion in the gamma-ray binary HESS J1832-093 as an O6 V star
DOI: 10.1093/mnrasl/slae007 Bibcode: 2024MNRAS.529L.102V

Papitto, A.; Negueruela, I.; de Oña Wilhelmi, E. +3 more

HESS J1832-093 is a member of the rare class of gamma-ray binaries, as recently confirmed by the detection of orbitally modulated X-ray and gamma-ray emission with a period of ~86 d. The spectral type of the massive companion star has been difficult to retrieve as there is no optical counterpart, but the system is coincident with a near-infrared s…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 3