Search Publications

Systematic Study of AGN Clumpy Tori with Broadband X-Ray Spectroscopy: Updated Unified Picture of AGN Structure
DOI: 10.3847/1538-4357/abccce Bibcode: 2021ApJ...906...84O

Tanimoto, Atsushi; Ueda, Yoshihiro; Ogawa, Shoji +1 more

We present the results of a systematic, broadband X-ray spectral analysis of nearby active galactic nuclei (AGNs) with the X-ray clumpy torus model (XCLUMPY). By adding 16 AGNs newly analyzed in this paper, we study a total of 28 AGNs, including unabsorbed and absorbed AGNs taken from Ichikawa et al. and García-Bernete et al. This is the largest s…

2021 The Astrophysical Journal
XMM-Newton 40
Multiple Stellar Populations along the Red Horizontal Branch and Red Clump of Globular Clusters
DOI: 10.3847/1538-4357/abc882 Bibcode: 2021ApJ...906...76D

Milone, A. P.; Cordoni, G.; Marino, A. F. +5 more

We exploit multiband Hubble Space Telescope photometry to investigate multiple populations (MPs) along the red horizontal branches (HBs) and red clumps of 14 metal-rich globular clusters (GCs), including 12 Milky Way GCs and the Magellanic Cloud GCs NGC 1978 and NGC 416. Based on appropriate two-color diagrams, we find that the fraction of first-g…

2021 The Astrophysical Journal
Gaia eHST 39
Compton-thick AGN in the NuSTAR Era VI: The Observed Compton-thick Fraction in the Local Universe
DOI: 10.3847/1538-4357/ac1c73 Bibcode: 2021ApJ...922..252T

Vignali, C.; Gilli, R.; Comastri, A. +11 more

We present the analysis of simultaneous Nuclear Spectroscopic Telescope Array (NuSTAR) and XMM-Newton data of eight Compton-thick active galactic nuclei (CT-AGN) candidates selected in the Swift-BAT 100 month catalog. This work is part of an ongoing effort to find and characterize all CT-AGN in the Local (z ≤ 0.05) Universe. We used two physically…

2021 The Astrophysical Journal
XMM-Newton 39
The Hawaii Infrared Parallax Program. V. New T-dwarf Members and Candidate Members of Nearby Young Moving Groups
DOI: 10.3847/1538-4357/abe3fa Bibcode: 2021ApJ...911....7Z

Siverd, Robert J.; Dupuy, Trent J.; Liu, Michael C. +2 more

We present a search for new planetary-mass members of nearby young moving groups (YMGs) using astrometry for 694 T and Y dwarfs, including 447 objects with parallaxes, mostly produced by recent large parallax programs from UKIRT and Spitzer. Using the BANYAN Σ and LACEwING algorithms, we identify 30 new candidate YMG members, with spectral types o…

2021 The Astrophysical Journal
Gaia 39
Outflows from Super Star Clusters in the Central Starburst of NGC 253
DOI: 10.3847/1538-4357/abec84 Bibcode: 2021ApJ...912....4L

Meier, David S.; Ott, Jürgen; Lenkić, Laura +13 more

Young massive clusters play an important role in the evolution of their host galaxies, and feedback from the high-mass stars in these clusters can have profound effects on the surrounding interstellar medium. The nuclear starburst in the nearby galaxy NGC 253 at a distance of 3.5 Mpc is a key laboratory in which to study star formation in an extre…

2021 The Astrophysical Journal
eHST 39
Observational Signature of Tightly Wound Spirals Driven by Buoyancy Resonances in Protoplanetary Disks
DOI: 10.3847/1538-4357/abe45e Bibcode: 2021ApJ...912...56B

Bae, Jaehan; Teague, Richard; Zhu, Zhaohuan

Besides the spirals induced by the Lindblad resonances, planets can generate a family of tightly wound spirals through buoyancy resonances. The excitation of buoyancy resonances depends on the thermal relaxation timescale of the gas. By computing timescales of various processes associated with thermal relaxation, namely, radiation, diffusion, and …

2021 The Astrophysical Journal
Gaia 39
A Population of Heavily Reddened, Optically Missed Novae from Palomar Gattini-IR: Constraints on the Galactic Nova Rate
DOI: 10.3847/1538-4357/abeb75 Bibcode: 2021ApJ...912...19D

Soria, Roberto; Tinyanont, Samaporn; De, Kishalay +25 more

The nova rate in the Milky Way remains largely uncertain, despite its vital importance in constraining models of Galactic chemical evolution as well as understanding progenitor channels for Type Ia supernovae. The rate has been previously estimated to be in the range of ≈10-300 yr-1, either based on extrapolations from a handful of very…

2021 The Astrophysical Journal
Gaia 39
An Ab Initio Approach to Antiproton Modulation in the Inner Heliosphere
DOI: 10.3847/1538-4357/abd3a5 Bibcode: 2021ApJ...908..167E

Engelbrecht, N. Eugene; Moloto, K. D.

Recent advances in the detection of cosmic-ray (CR) antiproton intensities at Earth have the potential to provide valuable new insights in the search for dark matter. As such, a fuller understanding of the modulation of these particles due to the influence of the Sun is of vital importance. Valuable insights can be gained through the study of gala…

2021 The Astrophysical Journal
Ulysses 39
The Infrared Emission and Vigorous Star Formation of Low-redshift Quasars
DOI: 10.3847/1538-4357/abe404 Bibcode: 2021ApJ...910..124X

Ho, Luis C.; Zhuang, Ming-Yang; Shangguan, Jinyi +1 more

The star formation activity of the host galaxies of active galactic nuclei provides valuable insights into the complex interconnections between black hole growth and galaxy evolution. A major obstacle arises from the difficulty of estimating accurate star formation rates (SFRs) in the presence of a strong active galactic nucleus. Analyzing the 1-5…

2021 The Astrophysical Journal
Herschel eHST 39
A Complex Luminosity Function for the Anomalous Globular Clusters in NGC 1052-DF2 and NGC 1052-DF4
DOI: 10.3847/1538-4357/abdd29 Bibcode: 2021ApJ...909..179S

van Dokkum, Pieter; Shen, Zili; Danieli, Shany

NGC 1052-DF2 and NGC 1052-DF4 are ultradiffuse galaxies that have extremely low velocity dispersions, indicating that they have little or no dark matter. Both galaxies host anomalously luminous globular clusters (GCs), with a peak magnitude of their GC luminosity function (GCLF) that is ∼1.5 mag brighter than the near-universal value of MV

2021 The Astrophysical Journal
eHST 39