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The Spatial and Emission Properties of the Large [O III] Emission Nebula Near M31
DOI: 10.3847/1538-4357/acfe0d Bibcode: 2023ApJ...957...82F

Shull, J. Michael; Fesen, Robert A.; Kimeswenger, Stefan +8 more

Drechsler et al. reported the unexpected discovery of a 1.°5 long [O III] emission nebula 1.°2 southeast of the M31 nucleus. Here we present additional images of this large emission arc, called the Strottner-Drechsler-Sainty Object (SDSO), along with radial velocity and flux measurements from low-dispersion spectra. Independent sets of [O III] ima…

2023 The Astrophysical Journal
Gaia 3
3D Spectroscopy with GTC-MEGARA of the Triple AGN Candidate in SDSS J102700.40+174900.8
DOI: 10.3847/1538-4357/acce3e Bibcode: 2023ApJ...952...45B

Shen, Yue; Liu, Xin; Rodríguez-Espinosa, José Miguel +4 more

Triple-active galactic nucleus (AGN) systems are expected to be the result of the hierarchical model of galaxy formation. Since there are very few of them confirmed as such, we present the results of a new study of the triple AGN candidate SDSS J102700.40+174900.8 (center nucleus) through observations with the GTC-MEGARA Integral Field Unit. 1D an…

2023 The Astrophysical Journal
eHST 3
The Missing Link: Testing Galactic Chemical Evolution Models with the First Multi-isotopic Abundances in Solar Twin Stars
DOI: 10.3847/1538-4357/acea5f Bibcode: 2023ApJ...954..121C

Crossfield, Ian J. M.; Freedman, Richard; Lothringer, Joshua +3 more

We present the first isotopic abundances of both 13CO and C18O in solar twin stars and test the results against several galactic chemical evolution (GCE) models with different nucleosynthesis prescriptions. First, we compare M-band spectra from IRTF/iSHELL to synthetic spectra generated from custom solar atmosphere models usi…

2023 The Astrophysical Journal
Gaia 3
Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra
DOI: 10.3847/1538-4357/acc066 Bibcode: 2023ApJ...948...16K

Kim, Seung-Lee

A star's rotation rate is difficult to estimate without surface inhomogeneities such as dark or bright spots. This paper presents asteroseismic results to determine the rotation rates of δ Sct-type pulsating primary stars in two eclipsing binary systems, AB Cas and OO Dra. After removing the binarity-induced light variations from archival TESS dat…

2023 The Astrophysical Journal
Gaia 3
Hubble Space Telescope Proper Motion Measurements of Supernova Remnant N132D: Center of Expansion and Age
DOI: 10.3847/1538-4357/acb8b6 Bibcode: 2023ApJ...948...33B

Blair, William P.; Law, Charles J.; Morse, Jon A. +8 more

We present proper motion measurements of the oxygen-rich ejecta of the LMC supernova remnant N132D using two epochs of Hubble Space Telescope Advanced Camera for Surveys data spanning 16 years. The proper motions of 120 individual knots of oxygen-rich gas were measured and used to calculate a center of expansion (CoE) of α = 5h25m<…

2023 The Astrophysical Journal
eHST 3
Wrinkles in Time. I. Rapid Rotators Found in High-eccentricity Orbits
DOI: 10.3847/1538-4357/acff69 Bibcode: 2023ApJ...958...76R

Rampalli, Rayna; Curtis, Jason L.; Newton, Elisabeth R. +2 more

Recent space-based missions have ushered in a new era of observational astronomy, where high-cadence photometric light curves for thousands to millions of stars in the solar neighborhood can be used to test and apply stellar age-dating methods, including gyrochronology. Combined with precise kinematics, these data allow for powerful new insights i…

2023 The Astrophysical Journal
Gaia 3
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Forming Quadruple System with Continuum "Ribbons" and Intricate Outflows
DOI: 10.3847/2041-8213/acdddf Bibcode: 2023ApJ...952L...2L

Sanhueza, Patricio; Kwon, Woojin; Chen, Huei-Ru Vivien +31 more

One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations toward a forming quadruple protostellar system, G206.93-16.61E2, in the Orion B molecular cloud. ALMA 1.3 mm continuum emission reveals …

2023 The Astrophysical Journal
Herschel 3
O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
DOI: 10.3847/1538-4357/ace16a Bibcode: 2023ApJ...953..112F

Matsushita, Kyoko; Fukushima, Kotaro; Kobayashi, Shogo B.

Chemical elements in the hot medium permeating early-type galaxies, groups, and clusters make such objects an excellent laboratory for studying metal enrichment and cycling processes on the largest scales of the universe. Here, we report the analysis by the XMM-Newton Reflection Grating Spectrometer of 14 early-type galaxies, including the well-kn…

2023 The Astrophysical Journal
XMM-Newton 3
Building an Acceleration Ladder with Tidal Streams and Pulsar Timing
DOI: 10.3847/2041-8213/acba15 Bibcode: 2023ApJ...945L..32C

Craig, Peter; Chakrabarti, Sukanya; Sanderson, Robyn E. +1 more

We analyse stellar streams in action-angle coordinates combined with recent local direct acceleration measurements to provide joint constraints on the potential of our galaxy. Our stream analysis uses the Kullback-Leibler divergence with a likelihood analysis based on the two-point correlation function. We provide joint constraints from pulsar acc…

2023 The Astrophysical Journal
Gaia 3
XMM-Newton and INTEGRAL Observations of the Bright GRB 230307A: Vanishing of the Local Absorption and Limits on the Dust in the Magellanic Bridge
DOI: 10.3847/1538-4357/acf846 Bibcode: 2023ApJ...956...97M

Mereghetti, Sandro; Tiengo, Andrea; Salvaterra, Ruben +2 more

GRB 230307A is the second brightest gamma-ray burst detected in more than 50 years of observations and is located in the direction of the Magellanic Bridge. Despite its long duration, it is most likely the result of the merger of a compact binary ejected from a galaxy in the local universe (redshift z = 0.065). Our XMM-Newton observation of its af…

2023 The Astrophysical Journal
INTEGRAL XMM-Newton 3