Search Publications

Not So Heavy Metals: Black Hole Feedback Enriches the Circumgalactic Medium
DOI: 10.3847/1538-4357/ab3045 Bibcode: 2019ApJ...882....8S

Werk, Jessica K.; Pontzen, Andrew; Christensen, Charlotte +4 more

We examine the effects of supermassive black hole (SMBH) feedback on the circumgalactic medium (CGM) using a cosmological hydrodynamic simulation (ROMULUS25) and a set of four zoom-in “genetically modified” Milky-Way-mass galaxies sampling different evolutionary paths. By tracing the distribution of metals in the CGM, we show that O VI is a sensit…

2019 The Astrophysical Journal
eHST 31
Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. X. Optical Variability Characteristics
DOI: 10.3847/1538-4357/ab16e8 Bibcode: 2019ApJ...877...23L

Ho, Luis C.; Bian, Wei-Hao; Zhang, Zhi-Xiang +11 more

We compiled a sample of 73 active galactic nuclei (AGNs) with reverberation mapping (RM) observations from RM campaigns, including our ongoing campaign of monitoring super-Eddington accreting massive black holes (BHs). This sample covers a large range of BH mass ({M}\bullet ={10}6{--9} {M}), dimensionless accreti…

2019 The Astrophysical Journal
eHST 31
Quiescent Galaxy Size and Spectroscopic Evolution: Combining HSC Imaging and Hectospec Spectroscopy
DOI: 10.3847/1538-4357/aaf97d Bibcode: 2019ApJ...872...91D

Geller, Margaret J.; Utsumi, Yousuke; Damjanov, Ivana +3 more

We explore the relationships between size, stellar mass, and average stellar population age (indicated by D n 4000 indices) for a sample of ∼11,000 intermediate-redshift galaxies from the SHELS spectroscopic survey (Geller et al. 2014) augmented by high-resolution Subaru Telescope Hyper Suprime-Cam imaging. In the redshift interval 0.1…

2019 The Astrophysical Journal
eHST 31
NuStar Hard X-Ray View of Low-luminosity Active Galactic Nuclei: High-energy Cutoff and Truncated Thin Disk
DOI: 10.3847/1538-4357/aaf38b Bibcode: 2019ApJ...870...73Y

Ho, Luis C.; Younes, George; Yuan, Feng +5 more

We report the analysis of simultaneous XMM-Newton+Nuclear Spectroscopic Telescope Array (NuSTAR) observations of two low-luminosity active galactic nuclei (LLAGNs), NGC 3998 and NGC 4579. We do not detect any significant variability in either source over the ∼3 day length of the NuSTAR observations. The broadband 0.5-60 keV spectrum of NGC 3998 is…

2019 The Astrophysical Journal
XMM-Newton 30
Interpretation of Departure from the Broad-line Region Scaling in Active Galactic Nuclei
DOI: 10.3847/1538-4357/aaf396 Bibcode: 2019ApJ...870...84C

Czerny, Bożena; Panda, Swayamtrupta; Du, Pu +7 more

Most results of the reverberation monitoring of active galaxies showed a universal scaling of the time delay of the Hβ emission region with the monochromatic flux at 5100 Å, with very small dispersion. Such a scaling favored the dust-based formation mechanism of the broad-line region (BLR). Recent reverberation measurements showed that actually a …

2019 The Astrophysical Journal
eHST 30
A Panchromatic View of the Bulge Globular Cluster NGC 6569
DOI: 10.3847/1538-4357/ab07c4 Bibcode: 2019ApJ...874...86S

Dalessandro, E.; Salaris, M.; Saracino, S. +12 more

We used high-resolution optical Hubble Space Telescope/WFC3 and multiconjugate adaptive optics assisted GEMINI GeMS/Gemini South Adaptive Optics Imager observations in the near-infrared (NIR) to investigate the physical properties of the globular cluster (GC) NGC 6569 in the Galactic bulge. We have obtained the deepest purely NIR color-magnitude d…

2019 The Astrophysical Journal
eHST 30
Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars
DOI: 10.3847/1538-4357/ab48e2 Bibcode: 2019ApJ...886..154Y

Tian, Hao; Zhao, Gang; Wu, Yaqian +12 more

We characterize the kinematic and chemical properties of ∼3000 Sagittarius (Sgr) stream stars, including K-giants, M-giants, and blue horizontal branch stars (BHBs), selected from SEGUE-2, Large Sky Area Multi-Object Fibre Spectroscopic Telescope, and Sloan Digital Sky Survey separately in Integrals-of-Motion space. The orbit of the Sgr stream is …

2019 The Astrophysical Journal
Gaia 30
SN 2016coi (ASASSN-16fp): An Energetic H-stripped Core-collapse Supernova from a Massive Stellar Progenitor with Large Mass Loss
DOI: 10.3847/1538-4357/ab3e37 Bibcode: 2019ApJ...883..147T

Hurley, K.; Challis, P.; Stanek, K. Z. +26 more

We present comprehensive observations and analysis of the energetic H-stripped SN 2016coi (a.k.a. ASASSN-16fp), spanning the γ-ray through optical and radio wavelengths, acquired within the first hours to ∼420 days post explosion. Our observational campaign confirms the identification of He in the supernova (SN) ejecta, which we interpret to be ca…

2019 The Astrophysical Journal
INTEGRAL XMM-Newton 30
Finding the Brightest Cosmic Beacons in the Southern Hemisphere
DOI: 10.3847/1538-4357/ab510a Bibcode: 2019ApJ...887..268C

Grazian, Andrea; Boutsia, Konstantina; Amorin, Ricardo +6 more

The study of absorptions along the lines of sight to bright high-z QSOs is an invaluable cosmological tool that provides a wealth of information on the inter-/circum-galactic medium, dark matter, primordial elements, reionization, fundamental constants, and general relativity. Unfortunately, the number of bright (i ≲ 18) QSOs at z ≳ 2 in the south…

2019 The Astrophysical Journal
Gaia 30
Chemical Cartography. II. The Assembly History of the Galactic Stellar Halo Traced by Carbon-enhanced Metal-poor Stars
DOI: 10.3847/1538-4357/ab4791 Bibcode: 2019ApJ...885..102L

Beers, Timothy C.; Lee, Young Sun; Kim, Young Kwang

We present an analysis of the kinematic properties of stellar populations in the Galactic halo, making use of over 100,000 main-sequence turnoff (MSTO) stars observed in the Sloan Digital Sky Survey. After dividing the Galactic halo into an inner-halo region (IHR) and outer-halo region (OHR), based on the spatial variation of carbon-to-iron ratios…

2019 The Astrophysical Journal
Gaia 30