Search Publications

The CO2 absorption spectrum in the 2.3 µm transparency window by high sensitivity CRDS: (II) Self-absorption continuum
DOI: 10.1016/j.jqsrt.2016.09.003 Bibcode: 2017JQSRT.187...38M

Campargue, A.; Vasilchenko, S.; Mondelain, D. +2 more

The CO2 absorption continuum near 2.3 µm is determined for a series of sub atmospheric pressures (250-750 Torr) by high sensitivity Cavity Ring Down Spectroscopy. An experimental procedure consisting in injecting successively a gas flow of CO2 and synthetic air, keeping constant the gas pressure in the CRDS cell, has be…

2017 Journal of Quantitative Spectroscopy and Radiative Transfer
VenusExpress 12
A Multi-band Study of the Remarkable Jet in Quasar 4C+19.44
DOI: 10.3847/1538-4357/aa845c Bibcode: 2017ApJ...846..119H

Cheung, C. C.; Uchiyama, Y.; Siemiginowska, A. +14 more

We present arcsecond-resolution data in the radio, IR, optical, and X-ray for 4C+19.44 (=PKS 1354+195), the longest and straightest quasar jet with deep X-ray observations. We report results from radio images with half to one arcsecond angular resolution at three frequencies, plus Hubble Space Telescope and Spitzer data. The Chandra data allow us …

2017 The Astrophysical Journal
eHST 12
The 2013 February 17 Sunquake in the Context of the Active Region's Magnetic Field Configuration
DOI: 10.3847/1538-4357/aa8db6 Bibcode: 2017ApJ...849...40G

Guglielmino, S. L.; Green, L. M.; Valori, G. +3 more

Sunquakes are created by the hydrodynamic response of the lower atmosphere to a sudden deposition of energy and momentum. In this study, we investigate a sunquake that occurred in NOAA active region 11675 on 2013 February 17. Observations of the corona, chromosphere, and photosphere are brought together for the first time with a nonlinear force-fr…

2017 The Astrophysical Journal
SOHO 12
Comparison of CME and ICME Structures Derived from Remote-Sensing and In Situ Observations
DOI: 10.1007/s11207-017-1171-7 Bibcode: 2017SoPh..292..157B

Bothmer, V.; Mrotzek, N.

We present results from the comparison of the near-Sun and in situ analysis of two Earth-directed coronal mass ejections (CMEs) with different 3D orientations and solar source region characteristics. The CME on 14 July 2000, the so-called Bastille Day storm, a well-studied event, was observed from a single-point perspective by the Large Angle and …

2017 Solar Physics
SOHO 12
KDG218, a nearby ultra-diffuse galaxy
DOI: 10.1134/S1990341317040022 Bibcode: 2017AstBu..72..376K

Sharina, M. E.; Karachentsev, I. D.; Makarova, L. N. +1 more

We present properties of the low-surface-brightness galaxy KDG218 observed with the HST/ACS. The galaxy has a half-light (effective) diameter of ae = 47″ and a central surface brightness of SBV(0) = 24.m4/□″. The galaxy remains unresolved with the HST/ACS, which implies its distance of D > 13.1 Mpc and linear ef…

2017 Astrophysical Bulletin
eHST 12
Infrared dust bubble CS51 and its interaction with the surrounding interstellar medium
DOI: 10.1093/mnras/stx2290 Bibcode: 2017MNRAS.472.4750D

Tej, Anandmayee; Liu, Hong-Li; Liu, Tie +4 more

A multiwavelength investigation of the southern infrared dust bubble CS51 is presented in this paper. We probe the associated ionized, cold dust, molecular and stellar components. Radio continuum emission mapped at 610 and 1300 MHz, using the Giant Metrewave Radio Telescope, India, reveals the presence of three compact emission components (A, B, a…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 12
Climbing the cosmic ladder with stellar twins in RAVE with Gaia
DOI: 10.1093/mnras/stx1877 Bibcode: 2017MNRAS.472.2517J

Gilmore, G.; Munari, U.; Steinmetz, M. +17 more

We apply the twin method to determine parallaxes to 232 545 stars of the RAVE survey using the parallaxes of Gaia DR1 as a reference. To search for twins in this large data set, we apply the t-student stochastic neighbour embedding projection that distributes the data according to their spectral morphology on a two-dimensional map. From this map, …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 12
XMM-Newton and INTEGRAL view of the hard state of EXO 1745-248 during its 2015 outburst
DOI: 10.1051/0004-6361/201629731 Bibcode: 2017A&A...603A..39M

Stella, L.; de Martino, D.; Rea, N. +10 more

Context. Transient low-mass X-ray binaries (LMXBs) often show outbursts that typically last a few weeks and are characterized by a high X-ray luminosity (Lx ≈ 1036-1038 erg s-1), while most of the time they are found in X-ray quiescence (LX ≈ 1031-1033 erg s-1)…

2017 Astronomy and Astrophysics
INTEGRAL XMM-Newton 12
The PMA Catalogue: 420 million positions and absolute proper motions
DOI: 10.1093/mnras/stx812 Bibcode: 2017MNRAS.469..763A

Akhmetov, V. S.; Fedorov, P. N.; Velichko, A. B. +1 more

We present a catalogue that contains about 420 million absolute proper motions of stars. It was derived from the combination of positions from Gaia DR1 and 2MASS, with a mean difference of epochs of about 15 yr. Most of the systematic zonal errors inherent in the 2MASS Catalogue were eliminated before deriving the absolute proper motions. The abso…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 12
No Evidence for Feedback: Unexceptional Low-ionization Winds in Host Galaxies of Low Luminosity Active Galactic Nuclei at Redshift z ∼ 1
DOI: 10.3847/1538-4357/aa6fae Bibcode: 2017ApJ...841...83Y

Prochaska, J. Xavier; Faber, S. M.; Coil, Alison L. +6 more

We study winds in 12 X-ray AGN host galaxies at z∼ 1. We find, using the low-ionization Fe II λ2586 absorption in the stacked spectra, that the probability distribution function (PDF) of the centroid-velocity shift in AGNs has 50th (median), 16th, and 84th percentiles of (-87, -251, +86) km s-1 respectively. The PDF of the velocity disp…

2017 The Astrophysical Journal
eHST 12