Search Publications

Co-evolution of Extreme Star Formation and Quasars: Hints from Herschel and the Sloan Digital Sky Survey
DOI: 10.1088/0004-637X/811/1/58 Bibcode: 2015ApJ...811...58M

Yan, Haojing; Ma, Zhiyuan

Using the public data from the Herschel wide-field surveys, we study the far-infrared properties of optical-selected quasars from the Sloan Digital Sky Survey. Within the common area of ∼172 deg2 , we have identified the far-infrared counterparts for 354 quasars, among which 134 are highly secure detections in the Herschel 250 µ {…

2015 The Astrophysical Journal
Herschel XMM-Newton 31
A Pilot Deep Survey for X-Ray Emission from fuvAGB Stars
DOI: 10.1088/0004-637X/810/1/77 Bibcode: 2015ApJ...810...77S

Stute, M.; Sahai, R.; Sánchez Contreras, C. +1 more

We report the results of a pilot survey for X-ray emission from a newly discovered class of AGB stars with far-ultraviolet excesses (fuvAGB stars) using XMM-Newton and Chandra. We detected X-ray emission in three of six fuvAGB stars observed—the X-ray fluxes are found to vary in a stochastic or quasi-periodic manner on roughly hour-long timescales…

2015 The Astrophysical Journal
XMM-Newton 31
Properties of Polycyclic Aromatic Hydrocarbons in the Northwest Photon Dominated Region of NGC 7023. III. Quantifying the Traditional Proxy for PAH Charge and Assessing its Role
DOI: 10.1088/0004-637X/806/1/121 Bibcode: 2015ApJ...806..121B

Boersma, C.; Allamandola, L. J.; Bregman, J.

Polycyclic aromatic hydrocarbon (PAH) emission in the Spitzer/IRS spectral map of the northwest photon dominated region (PDR) in NGC 7023 is analyzed. Here, results from fitting the 5.2-14.5 µm spectrum at each pixel using exclusively PAH spectra from the NASA Ames PAH IR Spectroscopic Database (www.astrochem.org/pahdb/) and observed PAH ban…

2015 The Astrophysical Journal
eHST 30
The Arches Cluster: Extended Structure and Tidal Radius
DOI: 10.1088/0004-637X/813/1/27 Bibcode: 2015ApJ...813...27H

Hosek, Matthew W., Jr.; Lu, Jessica R.; Clarkson, William I. +3 more

At a projected distance of ∼26 pc from Sgr A*, the Arches cluster provides insight into star formation in the extreme Galactic center (GC) environment. Despite its importance, many key properties, such as the cluster’s internal structure and orbital history, are not well known. We present an astrometric and photometric study of the outer region of…

2015 The Astrophysical Journal
eHST 30
O2 Emission toward Orion H2 Peak 1 and the Role of FUV-illuminated C-shocks
DOI: 10.1088/0004-637X/806/2/227 Bibcode: 2015ApJ...806..227M

Kaufman, Michael J.; Melnick, Gary J.

Molecular oxygen (O2) has been the target of ground-based and space-borne searches for decades. Of the thousands of lines of sight surveyed, only those toward Rho Ophiuchus and Orion H2 Peak 1 have yielded detections of any statistical significance. The detection of the O2 NJ = 33-12

2015 The Astrophysical Journal
Herschel 30
First New Solar Models with OPAS Opacity Tables
DOI: 10.1088/2041-8205/813/2/L42 Bibcode: 2015ApJ...813L..42L

Salmon, S.; Turck-Chièze, S.; Le Pennec, M. +4 more

Stellar seismology appears more and more as a powerful tool for a better determination of the fundamental properties of solar-type stars. However, the particular case of the Sun is still challenging. For about a decade now, the helioseismic sound-speed determination has continued to disagree with the standard solar model (SSM) prediction, question…

2015 The Astrophysical Journal
SOHO 30
Band-9 ALMA Observations of the [N II] 122 µm Line and FIR Continuum in Two High-z galaxies.
DOI: 10.1088/0004-637X/806/2/260 Bibcode: 2015ApJ...806..260F

Sheth, Kartik; Falgarone, Edith; Nikola, Thomas +4 more

We present Atacama Large Millimeter Array (ALMA) observations of two high-redshift systems (SMMJ02399-0136 at z 1 ∼ 2.8 and the Cloverleaf QSO at z 1 ∼ 2.5) in their rest-frame 122 µm continuum (ν sky ∼ 650 GHz, λ sky ∼ 450 µm) and [N ii] 122 µm line emission. The continuum observations…

2015 The Astrophysical Journal
eHST 30
Hiding in Plain Sight: Record-breaking Compact Stellar Systems in the Sloan Digital Sky Survey
DOI: 10.1088/2041-8205/808/1/L32 Bibcode: 2015ApJ...808L..32S

Janz, Joachim; Forbes, Duncan A.; Romanowsky, Aaron J. +10 more

Motivated by the recent, serendipitous discovery of the densest known galaxy, M60-UCD1, we present two initial findings from a follow-up search, using the Sloan Digital Sky Survey, Subaru/Suprime-Cam, and Hubble Space Telescope imaging, and SOuthern Astrophysical Research (SOAR)/Goodman spectroscopy. The first object discovered, M59-UCD3, has a si…

2015 The Astrophysical Journal
eHST 30
Characterization of the Inner Knot of the Crab: The Site of the Gamma-Ray Flares?
DOI: 10.1088/0004-637X/811/1/24 Bibcode: 2015ApJ...811...24R

Weisskopf, Martin C.; Tennant, Allyn; Caraveo, Patrizia +18 more

A particularly intriguing recent result from γ-ray astronomy missions is the detection of powerful flares from the Crab Nebula, which challenges the current understanding of pulsar wind nebulae and acceleration mechanisms. To search for the production site(s) of these flares, we conducted a multi-wavelength observing campaign using Keck, the Hubbl…

2015 The Astrophysical Journal
eHST 30
Herschel Observations of Extra-ordinary Sources: Analysi sof the HIFI 1.2 THz Wide Spectral Survey toward Orion KL II. Chemical Implications
DOI: 10.1088/0004-637X/806/2/239 Bibcode: 2015ApJ...806..239C

Favre, C.; Bergin, E. A.; Crockett, N. R. +5 more

We present chemical implications arising from spectral models fit to the Herschel/HIFI spectral survey toward the Orion Kleinmann-Low nebula (Orion KL). We focus our discussion on the eight complex organics detected within the HIFI survey utilizing a novel technique to identify those molecules emitting in the hottest gas. In particular, we find th…

2015 The Astrophysical Journal
Herschel 30