Search Publications

Simultaneous Constraints on the Mass and Radius of Aql X-1 from Quiescence and X-Ray Burst Observations
DOI: 10.3847/1538-4357/aa7d0b Bibcode: 2017ApJ...845....8L

Chen, Li; Falanga, Maurizio; Li, Zhaosheng +2 more

The measurement of neutron star mass and radius is one of the most direct ways to distinguish between various dense matter equations of state. The mass and radius of accreting neutron stars hosted in low-mass X-ray binaries can be constrained by several methods, including photospheric radius expansion from type I X-ray bursts and from quiescent sp…

2017 The Astrophysical Journal
XMM-Newton 9
Signatures of Hot Molecular Hydrogen Absorption from Protoplanetary Disks. I. Non-thermal Populations
DOI: 10.3847/1538-4357/aa7fc1 Bibcode: 2017ApJ...846....6H

Loyd, R. O. Parke; Kruczek, Nicholas; France, Kevin +2 more

The environment around protoplanetary disks (PPDs) regulates processes that drive the chemical and structural evolution of circumstellar material. We perform a detailed empirical survey of warm molecular hydrogen (H2) absorption observed against H I-Lyα (Lyα: λ1215.67) emission profiles for 22 PPDs, using archival Hubble Space Telescope…

2017 The Astrophysical Journal
eHST 9
The Carnegie-Chicago Hubble Program: Discovery of the Most Distant Ultra-faint Dwarf Galaxy in the Local Universe
DOI: 10.3847/2041-8213/835/2/L27 Bibcode: 2017ApJ...835L..27L

Lee, Myung Gyoon; Jang, In Sung; Seibert, Mark +3 more

Ultra-faint dwarf galaxies (UFDs) are the faintest known galaxies, and due to their incredibly low surface brightness, it is difficult to find them beyond the Local Group. We report a serendipitous discovery of a UFD, Fornax UFD1, in the outskirts of NGC 1316, a giant galaxy in the Fornax cluster. The new galaxy is located at a projected radius of…

2017 The Astrophysical Journal
eHST 9
HST Detection of Extended Neutral Hydrogen in a Massive Elliptical at z = 0.4
DOI: 10.3847/2041-8213/aa88a2 Bibcode: 2017ApJ...846L..29Z

Zahedy, Fakhri S.; Chen, Hsiao-Wen; Rauch, Michael +1 more

We report the first detection of extended neutral hydrogen (H I) gas in the interstellar medium (ISM) of a massive elliptical galaxy beyond z∼ 0. The observations utilize the doubly lensed images of QSO HE 0047-1756 at {z}{QSO}=1.676 as absorption-line probes of the ISM in the massive ({M}{star}≈ {10}11 {M}⊙ <…

2017 The Astrophysical Journal
eHST 9
The Nuclear X-Ray Emission-line Structure in NGC 2992 Revealed by Chandra-HETGS
DOI: 10.3847/1538-4357/aa6d6a Bibcode: 2017ApJ...840..120M

Nowak, M. A.; Marshall, H. L.; Murphy, K. D.

We present the narrow emission-line structure revealed by a 135 ks Chandra observation of Seyfert galaxy NGC 2992, using the High Energy Transmission Grating Spectrometer. The source was observed in an historically low-flux state. Using a Bayesian Block search technique, we detected neutral Si Kα and S Kα fluorescence and two additional lines that…

2017 The Astrophysical Journal
Suzaku 9
Herschel Extreme Lensing Line Observations: [CII] Variations in Galaxies at Redshifts z=1-3
DOI: 10.3847/1538-4357/835/1/110 Bibcode: 2017ApJ...835..110M

Carilli, Chris; Papovich, Casey; Strauss, Michael A. +14 more

We observed the [C II] line in 15 lensed galaxies at redshifts 1 < z < 3 using HIFI on the Herschel Space Observatory and detected 14/15 galaxies at 3σ or better. High magnifications enable even modestly luminous galaxies to be detected in [C II] with Herschel. The [C II] luminosity in this sample ranges from 8 × 107 L

2017 The Astrophysical Journal
Herschel 9
Structure and Dynamics of Cool Flare Loops Observed by the Interface Region Imaging Spectrograph
DOI: 10.3847/1538-4357/aa7d4e Bibcode: 2017ApJ...845...30M

Heinzel, P.; Berlicki, A.; Liu, W. +1 more

Flare loops were well observed with the Interface Region Imaging Spectrograph (IRIS) during the gradual phase of two solar flares on 2014 March 29 and 2015 June 22. Cool flare loops are visible in various spectral lines formed at chromospheric and transition-region temperatures and exhibit large downflows which correspond to the standard scenario.…

2017 The Astrophysical Journal
IRIS 9
The Stochastic X-Ray Variability of the Accreting Millisecond Pulsar MAXI J0911-655
DOI: 10.3847/1538-4357/aa607f Bibcode: 2017ApJ...837...61B

Bult, Peter

In this work, I report on the stochastic X-ray variability of the 340 Hz accreting millisecond pulsar MAXI J0911-655. Analyzing pointed observations of the XMM-Newton and NuSTAR observatories, I find that the source shows broad band-limited stochastic variability in the 0.01{--}10 {Hz} range with a total fractional variability of ∼ 24 % rms in the…

2017 The Astrophysical Journal
XMM-Newton 9
Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 < z < 2.7
DOI: 10.3847/1538-4357/aa6037 Bibcode: 2017ApJ...838...57K

Muzzin, Adam; Labbé, Ivo; Quadri, Ryan +13 more

We present the results of a pilot near-infrared spectroscopic campaign of five very massive galaxies ({log}({M}\star /{M})> 11.45) in the range of 1.7< z< 2.7. We measure an absorption feature redshift for one galaxy at {z}{spec}=2.000+/- 0.006. For the remaining galaxies, we combine the photometry with …

2017 The Astrophysical Journal
eHST 9
Propagation and Interaction Properties of Successive Coronal Mass Ejections in Relation to a Complex Type II Radio Burst
DOI: 10.3847/1538-4357/aa9075 Bibcode: 2017ApJ...849..112L

Liu, Ying D.; Zhao, Xiaowei; Zhu, Bei

We examine the propagation and interaction properties of three successive coronal mass ejections (CMEs) from 2001 November 21-22, with a focus on their connection with the behaviors of the associated long-duration complex type II radio burst. In combination with coronagraph and multi-point in situ observations, the long-duration type II burst prov…

2017 The Astrophysical Journal
SOHO Ulysses 9