Search Publications

Discovery of an X-Ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524
DOI: 10.3847/1538-4357/ab4ef8 Bibcode: 2019ApJ...887...69S

Veilleux, Sylvain; Tombesi, Francesco; Lohfink, Anne M. +2 more

We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524, which is classified as an ultraluminous infrared galaxy and optical Seyfert 2 at z = 0.0426. We test a variety of spectral models that yield a best fit consisting of an absorbed power law with emission and absorption features in the Fe K band. Remarkably, we f…

2019 The Astrophysical Journal
XMM-Newton 28
Modeling Mg II During Solar Flares. I. Partial Frequency Redistribution, Opacity, and Coronal Irradiation
DOI: 10.3847/1538-4357/ab3c24 Bibcode: 2019ApJ...883...57K

Kerr, Graham S.; Carlsson, Mats; Allred, Joel C.

The Interface Region Imaging Spectrograph has routinely observed the flaring Mg II near-ultraviolet (NUV) spectrum, offering excellent diagnostic potential and a window into the location of energy deposition. A number of studies have forward-modeled both the general properties of these lines and specific flare observations. Generally these have fo…

2019 The Astrophysical Journal
IRIS 28
Characteristics of the Two Sequences Seen in the High-velocity Hertzsprung-Russell Diagram in Gaia DR2
DOI: 10.3847/2041-8213/ab321e Bibcode: 2019ApJ...881L..10S

Casagrande, Luca; Feltzing, Sofia; Sahlholdt, Christian L.

In this study we use a sample of about 9 million SkyMapper stars with metallicities to investigate the properties of the two stellar populations seen in the high-velocity (V T > 200 km s-1) Gaia DR2 Hertzsprung-Russell diagram. Based on 10,000 red giant branch (RGB) stars (out of 75,000 with high velocity), we find that th…

2019 The Astrophysical Journal
Gaia 28
The Nitrogen Carrier in Inner Protoplanetary Disks
DOI: 10.3847/1538-4357/ab05d8 Bibcode: 2019ApJ...874...92P

Banzatti, Andrea; Walsh, Catherine; Pontoppidan, Klaus M. +4 more

The dominant reservoirs of elemental nitrogen in protoplanetary disks have not yet been observationally identified. Likely candidates are HCN, NH3, and N2. The relative abundances of these carriers determine the composition of planetesimals as a function of disk radius due to strong differences in their volatility. A signific…

2019 The Astrophysical Journal
Gaia 27
Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter/Submillimeter Cold Molecular Outflows in Seyfert Galaxies
DOI: 10.3847/1538-4357/aaf814 Bibcode: 2019ApJ...871..156M

Kohno, Kotaro; Mizumoto, Misaki; Izumi, Takuma

UltraFast Outflows (UFOs), seen as X-ray blueshifted absorption lines in active galactic nuclei (AGNs), are considered to be a key mechanism for AGN feedback. In this scenario, UFO kinetic energy is transferred into the cold and extended molecular outflow observed at the millimeter/submillimeter wavelength, which blows away the gas and suppresses …

2019 The Astrophysical Journal
Suzaku XMM-Newton 27
The Green Bank Ammonia Survey: A Virial Analysis of Gould Belt Clouds in Data Release 1
DOI: 10.3847/1538-4357/ab0c08 Bibcode: 2019ApJ...874..147K

Caselli, Paola; Chen, Mike; Di Francesco, James +14 more

We perform a virial analysis of starless dense cores in three nearby star-forming regions: L1688 in Ophiuchus, NGC 1333 in Perseus, and B18 in Taurus. Our analysis takes advantage of comprehensive kinematic information for the dense gas in all of these regions made publicly available through the Green Bank Ammonia Survey Data Release 1, which is u…

2019 The Astrophysical Journal
Herschel 27
Large-amplitude Quasiperiodic Pulsations as Evidence of Impulsive Heating in Hot Transient Loop Systems Detected in the EUV with SDO/AIA
DOI: 10.3847/1538-4357/ab4270 Bibcode: 2019ApJ...884..131R

Testa, Paola; Petralia, Antonino; Reale, Fabio +1 more

Short heat pulses can trigger plasma pressure fronts inside closed magnetic tubes in the corona. The alternation of condensations and rarefactions from the pressure modes drive large-amplitude pulsations in the plasma emission. Here we show the detection of such pulsations along magnetic tubes that brighten transiently in the hot 94 Å EUV channel …

2019 The Astrophysical Journal
IRIS 27
How Comets Work
DOI: 10.3847/2041-8213/ab2898 Bibcode: 2019ApJ...879L...8F

Blum, J.; Fulle, M.; Rotundi, A.

Two major questions regarding comets have been up to now far from any solution. (i) How is it possible that water-ice sublimation from the nucleus surface does not lead to an insulating crust, stopping every gas and dust ejection within a few days? (ii) How is it possible that the gas flow crossing the refractory surface crust ejects dust particle…

2019 The Astrophysical Journal
Rosetta 27
Red and Reddened: Ultraviolet through Near-infrared Observations of Type Ia Supernova 2017erp
DOI: 10.3847/1538-4357/ab1a3f Bibcode: 2019ApJ...877..152B

Wang, Lifan; Hsiao, E. Y.; Ruiter, Ashley J. +22 more

We present space-based ultraviolet/optical photometry and spectroscopy with the Swift Ultra-Violet/Optical Telescope and Hubble Space Telescope (HST), respectively, along with ground-based optical photometry and spectroscopy and near-infrared spectroscopy of supernova SN 2017erp. The optical light curves and spectra are consistent with a normal SN…

2019 The Astrophysical Journal
eHST 27
Calibrating Mg II-based Black Hole Mass Estimators with Hβ Reverberation Measurements
DOI: 10.3847/1538-4357/ab100d Bibcode: 2019ApJ...875...50B

Park, Daeseong; Woo, Jong-Hak; Bahk, Hyeonguk

We present the new calibration of black hole mass ({M}BH}) estimators based on the Mg II λ2798 broad emission line using the Hβ reverberation-mapped (RM) sample of 31 active galactic nuclei (AGNs) that have high-quality UV spectra. The updated and enlarged sample at redshift z < 0.16 covers a large dynamic range in {M}BH} …

2019 The Astrophysical Journal
IUE eHST 27