Search Publications

The PAH Emission Characteristics of the Reflection Nebula NGC 2023
DOI: 10.3847/1538-4357/836/2/198 Bibcode: 2017ApJ...836..198P

Wolfire, Mark G.; Peeters, Els; Tielens, Alexander G. G. M. +3 more

We present 5-20 µm spectral maps of the reflection nebula NGC 2023 obtained with the Infrared Spectrograph SL and SH modes on board the Spitzer Space Telescope, which reveal emission from polycyclic aromatic hydrocarbons (PAHs), C60, and H2 superposed on a dust continuum. We show that several PAH emission bands correlat…

2017 The Astrophysical Journal
ISO 84
Detection of Supermassive Black Holes in Two Virgo Ultracompact Dwarf Galaxies
DOI: 10.3847/1538-4357/aa6972 Bibcode: 2017ApJ...839...72A

Romanowsky, Aaron J.; Neumayer, Nadine; Strader, Jay +13 more

We present the detection of supermassive black holes (BHs) in two Virgo ultracompact dwarf galaxies (UCDs), VUCD3 and M59cO. We use adaptive optics assisted data from the Gemini/NIFS instrument to derive radial velocity dispersion profiles for both objects. Mass models for the two UCDs are created using multi-band Hubble Space Telescope imaging, i…

2017 The Astrophysical Journal
eHST 84
Estimating stellar atmospheric parameters, absolute magnitudes and elemental abundances from the LAMOST spectra with Kernel-based principal component analysis
DOI: 10.1093/mnras/stw2523 Bibcode: 2017MNRAS.464.3657X

Huang, Y.; Chen, B. -Q.; Wang, C. +16 more

Accurate determination of stellar atmospheric parameters and elemental abundances is crucial for Galactic archaeology via large-scale spectroscopic surveys. In this paper, we estimate stellar atmospheric parameters - effective temperature Teff, surface gravity log g and metallicity [Fe/H], absolute magnitudes MV and MKs<…

2017 Monthly Notices of the Royal Astronomical Society
Hipparcos 84
The WISSH quasars project. III. X-ray properties of hyper-luminous quasars
DOI: 10.1051/0004-6361/201731314 Bibcode: 2017A&A...608A..51M

Fiore, F.; Bianchi, S.; Martocchia, S. +14 more

We performed a survey of the X-ray properties of 41 objects from the WISE/SDSS selected hyper-luminous (WISSH) quasars sample, which includes 86 broad-line quasars with bolometric luminosity LBol ≳ 2 × 1047 erg s-1 shining at z 2-4. We used both proprietary and archival Chandra and XMM-Newton observations. Twenty-o…

2017 Astronomy and Astrophysics
XMM-Newton 84
A Spatially Resolved Study of Cold Dust, Molecular Gas, H II Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1
DOI: 10.3847/1538-4357/aa863a Bibcode: 2017ApJ...846..108C

Ivison, R. J.; Smail, Ian; Brandt, W. N. +17 more

We present detailed studies of a z = 2.12 submillimeter galaxy, ALESS67.1, using sub-arcsecond resolution ALMA, adaptive optics-aided VLT/SINFONI, and Hubble Space Telescope (HST)/CANDELS data to investigate the kinematics and spatial distributions of dust emission (870 µm continuum), 12CO(J = 3-2), strong optical emission lines, …

2017 The Astrophysical Journal
eHST 84
The relation between the column density structures and the magnetic field orientation in the Vela C molecular complex
DOI: 10.1051/0004-6361/201730608 Bibcode: 2017A&A...603A..64S

Ade, P. A. R.; Martin, P. G.; Netterfield, C. B. +27 more

We statistically evaluated the relative orientation between gas column density structures, inferred from Herschel submillimetre observations, and the magnetic field projected on the plane of sky, inferred from polarized thermal emission of Galactic dust observed by the Balloon-borne Large-Aperture Submillimetre Telescope for Polarimetry (BLASTPol)…

2017 Astronomy and Astrophysics
Herschel Planck 84
Astrometric Search Method for Individually Resolvable Gravitational Wave Sources with Gaia
DOI: 10.1103/PhysRevLett.119.261102 Bibcode: 2017PhRvL.119z1102M

Gilmore, Gerard; Mihaylov, Deyan P.; Moore, Christopher J. +1 more

Gravitational waves (GWs) cause the apparent position of distant stars to oscillate with a characteristic pattern on the sky. Astrometric measurements (e.g., those made by Gaia) provide a new way to search for GWs. The main difficulty facing such a search is the large size of the data set; Gaia observes more than one billion stars. In this Letter …

2017 Physical Review Letters
Gaia 84
Remote detection of widespread indigenous water in lunar pyroclastic deposits
DOI: 10.1038/ngeo2993 Bibcode: 2017NatGe..10..561M

Milliken, Ralph E.; Li, Shuai

Laboratory analyses of lunar samples provide a direct means to identify indigenous volatiles and have been used to argue for the presence of Earth-like water content in the lunar interior. Some volatile elements, however, have been interpreted as evidence for a bulk lunar mantle that is dry. Here we demonstrate that, for a number of lunar pyroclas…

2017 Nature Geoscience
Chandrayaan-1 84
The search for multiple populations in Magellanic Cloud clusters - II. The detection of multiple populations in three intermediate-age SMC clusters
DOI: 10.1093/mnras/stw3084 Bibcode: 2017MNRAS.465.4159N

Dalessandro, E.; Salaris, M.; Larsen, S. +14 more

This is the second paper in our series about the search for multiple populations in Magellanic Cloud star clusters using the Hubble Space Telescope. Here we report the detection of multiple stellar populations in the colour-magnitude diagrams of the intermediate-age clusters Lindsay 1, NGC 416 and NGC 339. With ages between 6.0 and 7.5 Gyr, these …

2017 Monthly Notices of the Royal Astronomical Society
eHST 83
Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy. II. Methods and Models
DOI: 10.3847/1538-4365/aa6b59 Bibcode: 2017ApJS..230....6K

Savage, Blair D.; Shull, J. Michael; Danforth, Charles W. +6 more

We present basic data and modeling for a survey of the cool, photoionized circumgalactic medium (CGM) of low-redshift galaxies using far-UV QSO absorption-line probes. This survey consists of “targeted” and “serendipitous” CGM subsamples, originally described in Stocke et al. (Paper I). The targeted subsample probes low-luminosity, late-type galax…

2017 The Astrophysical Journal Supplement Series
eHST 83