Search Publications

An Analysis of the Shapes of Interstellar Extinction Curves. VIII. The Optical Extinction Structure
DOI: 10.3847/1538-4357/ab6f01 Bibcode: 2020ApJ...891...67M

Gordon, Karl D.; Fitzpatrick, E. L.; Massa, Derck

New Hubble Space Telescope/STIS optical spectra were obtained for a sample of early-type stars with existing International Ultraviolet Explorer UV spectra. These data were used to construct optical extinction curves whose general properties are discussed elsewhere. In this paper, we identify extinction features in the curves that are wider than di…

2020 The Astrophysical Journal
eHST 20
On the Chemical and Kinematic Consistency between N-rich Metal-poor Field Stars and Enriched Populations in Globular Clusters
DOI: 10.3847/1538-4357/ab7233 Bibcode: 2020ApJ...891...28T

Shi, Jianrong; Fernández-Trincado, J. G.; Gao, Qi +5 more

Interesting chemically peculiar field stars may reflect their stellar evolution history and their possible origin in a different environment from where they are found now; this is one of the most important research fields in Galactic archeology. To explore this further, we have used the CN-CH bands around 4000 Å to identify N-rich metal-poor field…

2020 The Astrophysical Journal
Gaia 20
Increasing Activity in T CrB Suggests Nova Eruption Is Impending
DOI: 10.3847/2041-8213/abbb2c Bibcode: 2020ApJ...902L..14L

Sokoloski, J. L.; Mukai, Koji; Luna, Gerardo J. M. +1 more

Estimates of the accretion rate in symbiotic recurrent novae (RNe) often fall short of theoretical expectations by orders of magnitude. This apparent discrepancy can be resolved if the accumulation of mass by the white dwarf (WD) is highly sporadic, and most observations are performed during low states. Here we use a re-analysis of archival data f…

2020 The Astrophysical Journal
Gaia 20
Calibrating Mg II-based Black Hole Mass Estimators Using Low-to-high-luminosity Active Galactic Nuclei
DOI: 10.3847/1538-4357/abada0 Bibcode: 2020ApJ...901...35L

Xue, Yongquan; Woo, Jong-Hak; Le, Huynh Anh N.

We present single-epoch black hole mass (MBH) estimators based on the rest-frame ultraviolet (UV) Mg II 2798 Å and optical Hβ 4861 Å emission lines. To enlarge the luminosity range of active galactic nuclei (AGNs), we combine the 31 reverberation-mapped AGNs with relatively low luminosities from Bahk et al., 47 moderate-luminosity AGNs …

2020 The Astrophysical Journal
eHST 20
Discovery of Magellanic Stellar Debris in the H3 Survey
DOI: 10.3847/2041-8213/abcb83 Bibcode: 2020ApJ...905L...3Z

Conroy, Charlie; Ting, Yuan-Sen; Cargile, Phillip A. +9 more

We report the discovery of 15 stars in the H3 survey that lie, in projection, near the tip of the trailing gaseous Magellanic Stream (MS). The stars have Galactocentric velocities <-155 km s-1, Galactocentric distances of ≈40 to 80 kpc (increasing along the MS), and [Fe/H] consistent with that of stars in the Small Magellanic Cloud. …

2020 The Astrophysical Journal
Gaia 20
Luminous Lyα Emitters with Very Blue UV-continuum Slopes at Redshift 5.7 ≤ z ≤ 6.6
DOI: 10.3847/1538-4357/ab64ea Bibcode: 2020ApJ...889...90J

Jiang, Linhua; Schaerer, Daniel; Egami, Eiichi +4 more

We study six luminous Lyα emitters (LAEs) with very blue rest-frame UV continua at 5.7 ≤ z ≤ 6.6. These LAEs have previous Hubble Space Telescope (HST) and Spitzer IRAC observations. Combining our newly acquired HST images, we find that their UV-continuum slopes β are in a range of -3.4 ≤ β ≤ -2.6. Unlike previous, tentative detections of β ≃ -3 i…

2020 The Astrophysical Journal
eHST 20
The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars
DOI: 10.3847/1538-4357/ab97ba Bibcode: 2020ApJ...898...40C

Beers, Timothy C.; Placco, Vinicius M.; Hattori, Kohei +8 more

We report the discovery of J1521-3538, a bright (V = 12.2), very metal-poor ([Fe/H] = -2.8) strongly r-process-enhanced field horizontal branch star, based on a high-resolution, high signal-to-noise Magellan/MIKE spectrum. J1521-3538 shows the largest r-process element overabundance in any known r-process-enhanced star, with [Eu/Fe] = +2.2, and it…

2020 The Astrophysical Journal
Gaia 20
The Accretion History of AGN: A Newly Defined Population of Cold Quasars
DOI: 10.3847/1538-4357/aba358 Bibcode: 2020ApJ...900....5K

Kartaltepe, Jeyhan S.; Kirkpatrick, Allison; Marchesi, Stefano +15 more

Quasars are the most luminous of active galactic nuclei, and are perhaps responsible for quenching star formation in their hosts. The Stripe 82X catalog covers 31.3 deg2 of the Stripe 82 field, of which the 15.6 deg2 covered with XMM-Newton is also covered by Herschel/SPIRE. We have 2500 X-ray detected sources with multiwavel…

2020 The Astrophysical Journal
Herschel XMM-Newton 20
The Population of Galactic Planetary Nebulae: a Study of Distance Scales and Central Stars Based on the Second Gaia Release
DOI: 10.3847/1538-4357/ab59e4 Bibcode: 2020ApJ...889...21S

Stanghellini, Letizia; Bucciarelli, Beatrice; Lattanzi, Mario G. +1 more

We matched the astrometry of central stars (CSs) of spectroscopically confirmed Galactic planetary nebulae (PNe) with DR2 Gaia parallaxes (p), finding 430 targets in common with p > 0 and $| {\sigma }_{{\rm{p}}}/p| \lt 1$ ∣ σ p / p ∣ < 1 . A catalog of PNe whose CSs have DR2 Gaia parallaxes is presented in Table 1. We compared DR2 parallaxes…

2020 The Astrophysical Journal
Gaia 20
Hot Subdwarf Stars Identified in Gaia DR2 with Spectra of LAMOST DR6 and DR7. II.Kinematics
DOI: 10.3847/1538-4357/ab98f3 Bibcode: 2020ApJ...898...64L

Luo, Yangping; Németh, Péter; Li, Qida

Combining LAMOST radial velocities with Gaia parallaxes and proper motions, we present 3D Galactic space motions and the orbits of 182 single-lined hot subdwarf stars. These stars were identified by Lei et al. in Gaia DR2 with LAMOST DR6 and DR7 spectra. He-rich hot subdwarf stars with $\mathrm{log}(y)\geqslant 0$ show the largest standard deviati…

2020 The Astrophysical Journal
Gaia 19