Search Publications

A Herschel/HIFI Legacy Survey of HF and H2O in the Galaxy: Probing Diffuse Molecular Cloud Chemistry
DOI: 10.1088/0004-637X/806/1/49 Bibcode: 2015ApJ...806...49S

Gerin, M.; Neufeld, D. A.; Sonnentrucker, P. +5 more

We combine Herschel observations for a total of 12 sources to construct the most uniform survey of HF and H2O in our Galactic disk. Both molecules are detected in absorption along all sight lines. The high spectral resolution of the Heterodyne Instrument for the Far-infrared (HIFI) allows us to compare the HF and H2O distribu…

2015 The Astrophysical Journal
Herschel 22
Redshifted Fe Kα line from the unusual γ-ray source PMN J1603-4904
DOI: 10.1051/0004-6361/201425442 Bibcode: 2015A&A...574A.117M

Stawarz, Ł.; Dauser, T.; Wilms, J. +13 more

Context. Multiwavelength observations have revealed the highly unusual properties of the γ-ray source PMN J1603-4904, which are difficult to reconcile with any other well-established γ-ray source class. The object is either a very atypical blazar or a compact jet source seen at a larger angle to the line of sight.
Aims: To determine the physi…

2015 Astronomy and Astrophysics
Suzaku XMM-Newton 22
The Relation between Dynamical Mass-to-light Ratio and Color for Massive Quiescent Galaxies out to z ~ 2 and Comparison with Stellar Population Synthesis Models
DOI: 10.1088/0004-637X/799/2/125 Bibcode: 2015ApJ...799..125V

van Dokkum, Pieter G.; Franx, Marijn; Bezanson, Rachel +2 more

We explore the relation between the dynamical mass-to-light ratio (M/L) and rest-frame color of massive quiescent galaxies out to z ~ 2. We use a galaxy sample with measured stellar velocity dispersions in combination with Hubble Space Telescope and ground-based multi-band photometry. Our sample spans a large range in log M dyn/L g…

2015 The Astrophysical Journal
eHST 22
Hunting for Orphaned Central Compact Objects among Radio Pulsars
DOI: 10.1088/0004-637X/808/2/130 Bibcode: 2015ApJ...808..130L

Ng, C. -Y.; Ho, W. C. G.; Bogdanov, S. +3 more

Central compact objects (CCOs) are a handful of young neutron stars found at the center of supernova remnants (SNRs). They show high thermal X-ray luminosities but no radio emission. Spin-down rate measurements of three CCOs with X-ray pulsations indicate surface dipole fields much weaker than those of typical young pulsars. To investigate if CCOs…

2015 The Astrophysical Journal
XMM-Newton 22
Craters on comets
DOI: 10.1016/j.pss.2014.06.008 Bibcode: 2015P&SS..107...53V

Vincent, Jean-Baptiste; Oklay, Nilda; Sierks, Holger +2 more

This paper reviews the observations of crater-like features on cometary nuclei. We compare potential crater sizes and morphologies, and we discuss the probability of impacts between small asteroids in the Main Belt and a comet crossing this region of the Solar System. Finally, we investigate the fate of the impactor and its chances of survival on …

2015 Planetary and Space Science
Rosetta 22
The First "Water Fountain" Collimated Outflow in a Planetary Nebula
DOI: 10.1088/0004-637X/799/2/186 Bibcode: 2015ApJ...799..186G

Bendjoya, Philippe; Guerrero, Martín A.; Ramos-Larios, Gerardo +8 more

"Water fountains" (WFs) are evolved objects showing high-velocity, collimated jets traced by water maser emission. Most of them are in the post-asymptotic giant branch (post-AGB) and they may represent one of the first manifestations of collimated mass loss in evolved stars. We present water maser, carbon monoxide, and mid-infrared spectroscopic d…

2015 The Astrophysical Journal
Herschel 22
Evidence for a [WR] or WEL-type binary nucleus in the bipolar planetary nebula Vy 1-2
DOI: 10.1093/mnras/stv1468 Bibcode: 2015MNRAS.452.2911A

Boumis, P.; López, J. A.; Akras, S. +3 more

We present high-dispersion spectroscopic data of the compact planetary nebula Vy 1-2, where high expansion velocities up to 100 km s-1 are found in the Hα, [N II] and [O III] emission lines. Hubble Space Telescope images reveal a bipolar structure. Vy 1-2 displays a bright ring-like structure with a size of 2.4 arcsec × 3.2 arcsec and t…

2015 Monthly Notices of the Royal Astronomical Society
AKARI eHST 22
The warm molecular gas and dust of Seyfert galaxies: two different phases of accretion?
DOI: 10.1093/mnras/stv1408 Bibcode: 2015MNRAS.452.4128M

Prieto, M. A.; Fernández-Ontiveros, J. A.; Neumayer, N. +3 more

The distribution of warm molecular gas (1000-3000 K), traced by the near-IR H2 2.12 µm line, has been imaged with a resolution <0.5 arcsec in the central 1 kpc of seven nearby Seyfert galaxies. We find that this gas is highly concentrated towards the central 100 pc and that its morphology is often symmetrical. Lanes of warm H

2015 Monthly Notices of the Royal Astronomical Society
eHST 21
Modeling the Chromosphere of a Sunspot and the Quiet Sun
DOI: 10.1088/0004-637X/811/2/87 Bibcode: 2015ApJ...811...87A

Curdt, W.; Tian, H.; Landi, E. +2 more

Semiempirical atmospheric modeling attempts to match an observed spectrum by finding the temperature distribution and other physical parameters along the line of sight through the emitting region such that the calculated spectrum agrees with the observed one. In this paper we take the observed spectrum of a sunspot and the quiet Sun in the EUV wav…

2015 The Astrophysical Journal
IRIS SOHO 21
A Determination of the North-South Heliospheric Magnetic Field Component from Inner Corona Closed-loop Propagation
DOI: 10.1088/2041-8205/803/1/L1 Bibcode: 2015ApJ...803L...1J

Jackson, B. V.; Buffington, A.; Hick, P. P. +4 more

A component of the magnetic field measured in situ near the Earth in the solar wind is present from north-south fields from the low solar corona. Using the Current-sheet Source Surface model, these fields can be extrapolated upward from near the solar surface to 1 AU. Global velocities inferred from a combination of interplanetary scintillation ob…

2015 The Astrophysical Journal
SOHO 21