Search Publications

Detections of Massive Stars in the Cluster MCM2005b77, in the Star-forming Regions GRS G331.34-00.36 (S62) and GRS G337.92-00.48 (S36)
DOI: 10.3847/1538-4357/aac6d4 Bibcode: 2018ApJ...862...10M

Menten, Karl M.; Rich, R. Michael; Figer, Donald F. +2 more

Large infrared and millimeter wavelength surveys of the Galactic plane have unveiled more than 600 new bubble H II regions and more than 3000 candidate star clusters. We present a study of the candidate clusters MCM2005b72, DBS2003-157, DBS2003-172, and MCM2005b77 based on near-infrared spectroscopy taken with SofI on the NTT and infrared photomet…

2018 The Astrophysical Journal
Gaia 3
The LABOCA/ACT Survey of Clusters at All Redshifts: Multiwavelength Analysis of Background Submillimeter Galaxies
DOI: 10.3847/1538-4357/aaaab0 Bibcode: 2018ApJ...855...26A

Hilton, Matt; Bond, J. Richard; Dünner, Rolando +12 more

We present a multiwavelength analysis of 48 submillimeter galaxies (SMGs) detected in the Large APEX Bolometer Camera/Atacama Cosmology Telescope (ACT) Survey of Clusters at All Redshifts, LASCAR, which acquired new 870 µm and Australia Telescope Compact Array 2.1 GHz observations of 10 galaxy clusters detected through their Sunyaev-Zel’dovi…

2018 The Astrophysical Journal
Herschel 3
Chromospheric Response during the Precursor and the Main Phase of a B6.4 Flare on 2005 August 20
DOI: 10.3847/1538-4357/aabd76 Bibcode: 2018ApJ...858...98A

Awasthi, Arun Kumar; Liu, Rui; Berlicki, Arkadiusz +2 more

Solar flare precursors depict a constrained rate of energy release, in contrast to the imminent rapid energy release, which calls for a different regime of plasma processes to be at play. Due to the subtle emission during the precursor phase, its diagnostics remain delusive, revealing either nonthermal electrons (NTEs) or thermal conduction to be …

2018 The Astrophysical Journal
SOHO 3
ALMA Observation of NGC 5135: The Circumnuclear CO (6-5) and Dust Continuum Emission at 45 pc Resolution
DOI: 10.3847/1538-4357/aae1f4 Bibcode: 2018ApJ...866..117C

Inami, Hanae; van der Werf, Paul; Gao, Yu +10 more

We present high-resolution (0.″17 × 0.″14) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO (6-5) line and 435 µm dust continuum emission within a ∼9″ × 9″ area centered on the nucleus of the galaxy NGC 5135. NGC 5135 is a well-studied luminous infrared galaxy that also harbors a Compton-thick active galactic nucleu…

2018 The Astrophysical Journal
eHST 3
Particles Co-orbital to Janus and to Epimetheus: A Firefly Planetary Ring
DOI: 10.3847/1538-4357/aa9c7f Bibcode: 2018ApJ...852...14W

Sfair, Rafael; Winter, Othon C.; Souza, Alexandre P. S. +3 more

The Cassini spacecraft found a new and unique ring that shares the trajectory of Janus and Epimetheus, co-orbital satellites of Saturn. Performing image analysis, we found this to be a continuous ring. Its width is between 30% and 50% larger than previously announced. We also verified that the ring behaves like a firefly. It can only be seen from …

2018 The Astrophysical Journal
Cassini 3
Evolution of the Outflows in NGC 3516
DOI: 10.3847/1538-4357/aaa95d Bibcode: 2018ApJ...854..166D

Kraemer, S. B.; Dunn, Jay P.; Parvaresh, Rozhin +1 more

We analyze the 2011 HST/COS spectrum of the Seyfert 1 galaxy NGC 3516, which demonstrates clear changes in one of the intrinsic absorption troughs (component 5), slight evidence of change in a second trough (component 6), and the appearance of a new absorption trough (component 9). We interpret both the changes and the appearance of the new trough…

2018 The Astrophysical Journal
IUE eHST 3
Dust Production Rates in the Fomalhaut Debris Disk from SOFIA/FORCAST Mid-infrared Imaging
DOI: 10.3847/1538-4357/aacf96 Bibcode: 2018ApJ...862..161A

Lau, R. M.; Herter, T. L.; Adams, J. D. +2 more

We present the first spatially resolved mid-infrared (37.1 µm) image of the Fomalhaut debris disk. We use point spread function fitting and subtraction to distinctly measure the flux from the unresolved component and the debris disk. We measure an infrared excess in the point source of 0.9 ± 0.2 Jy, consistent with emission from warm dust in…

2018 The Astrophysical Journal
Herschel 2
Ultraviolet Flux Decrease Under a Grand Minimum from IUE Short-wavelength Observation of Solar Analogs
DOI: 10.3847/2041-8213/aaa124 Bibcode: 2018ApJ...852L...4L

Melis, Carl; Tytler, David; Lubin, Dan

We have identified a sample of 33 Sun-like stars observed by the International Ultraviolet Explorer (IUE) with the short-wavelength spectrographs that have ground-based detections of chromospheric Ca II H+K activity. Our objective is to determine if these observations can provide an estimate of the decrease in ultraviolet (UV) surface flux associa…

2018 The Astrophysical Journal
IUE 2
Spatially Extended Low-ionization Emission Regions (LIERs) at z ∼ 0.9
DOI: 10.3847/1538-4357/aae690 Bibcode: 2018ApJ...868...16H

Marchesini, Danilo; Momcheva, Ivelina G.; Brammer, Gabriel B. +9 more

We present spatially resolved emission diagnostics for eight z ∼ 0.9 galaxies that demonstrate extended low-ionization emission line regions over kpc scales. Eight candidates are selected based on their spatial extent and emission line fluxes from slitless spectroscopic observations with the Hubble Space Telescope/Wide Field Camera 3 G141 and G800…

2018 The Astrophysical Journal
eHST 2
J0453-6655, the Supernova Remnant in N4D
DOI: 10.3847/1538-4357/aabf43 Bibcode: 2018ApJ...861..154S

Points, S. D.; Murray, S. S.; Smith, R. K. +4 more

The Large Magellanic Cloud supernova remnant J0453-6655 in the H II region N4 has been observed with XMM-Newton and with Chandra. Almost all of the diffuse X-ray emission is from within a 3.‧5 × 2.‧3 region of bright optical filaments, and X-ray results from XMM-Newton and Chandra are very similar. Spectra indicate that the plasma is close to equi…

2018 The Astrophysical Journal
XMM-Newton 2