Search Publications

CAHA/PPAK Integral-field Spectroscopic Observations of M81. II. Testing Photoionization Models in a Spatially Resolved LINER
DOI: 10.3847/1538-4357/ad0299 Bibcode: 2023ApJ...958...89L

Li, Zhiyuan; García-Benito, Rubén; Li, Zongnan +1 more

The origin of the low-ionization nuclear emission-line region (LINER) prevalent in local galaxies and its relationship with supermassive black holes have been debated for decades. We perform a comprehensive evaluation of traditional photoionization models against the circumnuclear ionized gas in M81, for which recent CAHA/PPAK integral-field spect…

2023 The Astrophysical Journal
eHST 0
Temporal Behaviors of Magnetic Helicity Injections by Self and Mutual Sunspot Rotations
DOI: 10.3847/1538-4357/aca800 Bibcode: 2023ApJ...943...96H

Shimizu, Toshifumi; Hasegawa, Takahiro

Magnetic helicity is a physical parameter used to quantify the complexity of magnetic fields, providing an indication of the energy state in the coronal magnetic structure. We investigate the temporal evolution of magnetic helicity and its relationship to the occurrence of a variety of flares in the solar active region NOAA 12297, which was well o…

2023 The Astrophysical Journal
SOHO 0
Sparse Logistic Regression for RR Lyrae versus Binaries Classification
DOI: 10.3847/1538-4357/accf8f Bibcode: 2023ApJ...950..103T

Bono, Giuseppe; Pasquato, Mario; Braga, Vittorio F. +4 more

RR Lyrae (RRL) stars are old, low-mass, radially pulsating variable stars in their core helium burning phase. They are popular stellar tracers and primary distance indicators since they obey well-defined period-luminosity relations in the near-infrared regime. Their photometric identification is not trivial; indeed, RRL star samples can be contami…

2023 The Astrophysical Journal
Gaia 0
A Survey for C II Emission-line Stars in the Large Magellanic Cloud. II. Final Results and the Origin of C II Emission in [WC] Spectra
DOI: 10.3847/1538-4357/aca8a6 Bibcode: 2023ApJ...942...85M

Massey, Philip; Morrell, Nidia; Neugent, Kathryn F. +2 more

We present the final results of an imaging and spectroscopic search for stars in the Large Magellanic Cloud (LMC) with C II λλ7231, 7236 emission lines. The goal is to identify and study [WC11] stars, the coolest of the low-mass Wolf-Rayet sequence, and a subset of central stars of planetary nebulae where the C II lines are known to be especially …

2023 The Astrophysical Journal
Gaia 0
Reconstructing the Volume Density Profile of Prestellar Cores with the Anisotropic Inverse Abel Transform Method
DOI: 10.3847/1538-4357/acd75e Bibcode: 2023ApJ...952...83Z

Zhang, Yapeng; Liu, Zhengdong; An, Weiming +2 more

Most studies of the 3D density structure of prestellar cores have used isotropic evolution models, which are projected into 2D for direct comparison with observation data. In this study, we introduced the anisotropic inverse Abel transform method for reconstructing the 3D volume density profile of prestellar cores. We demonstrated that this approa…

2023 The Astrophysical Journal
Herschel 0
Multiwavelength Study of Dark Globule DC 314.8-5.1: Point-source Identification and Diffuse Emission Characterization
DOI: 10.3847/1538-4357/ad077a Bibcode: 2023ApJ...959...37K

Cheung, C. C.; Stawarz, Ł.; Rocha, W. R. M. +3 more

We present an analysis of multiwavelength observations of the dark globule DC 314.8-5.1, using data from the Gaia optical, Two Micron All Star Survey near-infrared, and Wide-field Infrared Survey Explorer mid-infrared surveys, dedicated imaging with the Spitzer Space Telescope, and X-ray data obtained with the Swift X-Ray Telescope (XRT). The main…

2023 The Astrophysical Journal
Gaia 0
Electrostatic Plasma Wave Excitations at the Interplanetary Shocks
DOI: 10.3847/1538-4357/aca7c6 Bibcode: 2023ApJ...943...16S

Giacalone, Joe; Fraschetti, Federico; Singh, Manpreet

Over the last few decades, different types of plasma waves (e.g., the ion acoustic waves (IAWs), electrostatic solitary waves, upper/lower hybrid waves, and Langmuir waves) have been observed in the upstream, downstream, and ramp regions of the collisionless interplanetary (IP) shocks. These waves may appear as short-duration (only a few milliseco…

2023 The Astrophysical Journal
Ulysses 0
X-Ray Spectroscopy of Interstellar Carbon: Evidence for Scattering by Carbon-bearing Material in the Spectrum of 1ES 1553+113
DOI: 10.3847/1538-4357/acd0ab Bibcode: 2023ApJ...949...26S

Paerels, Frits; Staunton, John

Molecules and particles make up ~40%-70% of carbon in the interstellar medium, yet the exact chemical structure of these constituents remains unknown. We present carbon K-shell absorption spectroscopy of the Galactic interstellar medium obtained with the Low Energy Transmission Grating Spectrometer on board the Chandra Observatory that directly ad…

2023 The Astrophysical Journal
IUE 0
Near-infrared Polarimetry and H2 Emission toward Massive Young Stars: Discovery of a Bipolar Outflow Associated to S235 e2s3
DOI: 10.3847/1538-4357/acb68e Bibcode: 2023ApJ...944..226D

Ray, T. P.; Dewangan, L. K.; Luna, A. +3 more

We present a near-infrared H-band polarimetric study toward the S235 e2s3 protostar, obtained using the POLICAN instrument on the 2.1 m OAGH telescope. The images reveal a bipolar outflow with a total length of about 0.5 pc. The outflow nebulosity presents a high degree of linear polarization (~80%) and reveals a centrosymmetric pattern with the p…

2023 The Astrophysical Journal
AKARI Gaia 0
Discovery of an X-Ray Photoionized Optical Nebula and a Radio Nebula Associated with the ULX NGC 4861 X-1
DOI: 10.3847/1538-4357/acf8c3 Bibcode: 2023ApJ...958...24G

Liu, Jifeng; Gong, Hang; Urquhart, Ryan +5 more

We have conducted long-slit spectroscopic observations and analyzed archival radio data for the ultraluminous X-ray source (ULX) NGC 4861 X-1. Our spectral line analysis unveils NGC 4861 X-1 as the fourth ULX situated within an X-ray photoionized nebula, following three previous findings made approximately two decades ago. Remarkably, we discover …

2023 The Astrophysical Journal
eHST 0