Search Publications

Mixed aliphatic and aromatic composition of evaporating very small grains in NGC 7023 revealed by the 3.4/3.3 µm ratio
DOI: 10.1051/0004-6361/201425590 Bibcode: 2015A&A...577A..16P

Boulanger, F.; Joblin, C.; Onaka, T. +1 more

Context. A chemical scenario was proposed for photon-dominated regions (PDRs) according to which UV photons from nearby stars lead to the evaporation of very small grains (VSGs) and the production of gas-phase polycyclic aromatic hydrocarbons (PAHs).
Aims: Our goal is to achieve better insight into the composition and evolution of evaporating…

2015 Astronomy and Astrophysics
AKARI 68
XMM-Newton Survey of Local O VII Absorption Lines in the Spectra of Active Galactic Nuclei
DOI: 10.1088/0067-0049/217/2/21 Bibcode: 2015ApJS..217...21F

Fang, Taotao; Bullock, James; Buote, David +1 more

Highly ionized, z = 0 metal absorption lines detected in the X-ray spectra of background active galactic nuclei (AGNs) provide an effective method to probe the hot (T ∼ 106 K) gas and its metal content in and around the Milky Way. We present an all-sky survey of the {{K}α } transition of the local O vii absorption lines obtai…

2015 The Astrophysical Journal Supplement Series
XMM-Newton 68
Scientific assessment of the quality of OSIRIS images
DOI: 10.1051/0004-6361/201525985 Bibcode: 2015A&A...583A..46T

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +51 more

Context. OSIRIS, the scientific imaging system onboard the ESA Rosetta spacecraft, has been imaging the nucleus of comet 67P/Churyumov-Gerasimenko and its dust and gas environment since March 2014. The images serve different scientific goals, from morphology and composition studies of the nucleus surface, to the motion and trajectories of dust gra…

2015 Astronomy and Astrophysics
Rosetta 68
Determination of the Mass of IGR J17091-3624 from "Spectro-temporal" Variations during the Onset Phase of the 2011 Outburst
DOI: 10.1088/0004-637X/807/1/108 Bibcode: 2015ApJ...807..108I

Nandi, A.; Mandal, S.; Iyer, N.

The 2011 outburst of the black hole candidate IGR J17091-3624 followed the canonical track of state transitions along with the evolution of quasi-periodic oscillation (QPO) frequencies before it began exhibiting various variability classes similar to GRS 1915+105. We use this canonical evolution of spectral and temporal properties to determine the…

2015 The Astrophysical Journal
INTEGRAL 68
Herschel-ATLAS: the connection between star formation and AGN activity in radio-loud and radio-quiet active galaxies
DOI: 10.1093/mnras/stv1502 Bibcode: 2015MNRAS.452.3776G

Ivison, R. J.; Fritz, J.; Hardcastle, M. J. +6 more

We examine the relationship between star formation and active galactic nuclei (AGN) activity by constructing matched samples of local (0 < z < 0.6) radio-loud and radio-quiet AGN in the Herschel-Astrophysical Terahertz Large Area Survey fields. Radio-loud AGN are classified as high-excitation and low-excitation radio galaxies using their emi…

2015 Monthly Notices of the Royal Astronomical Society
Herschel 68
Signals of a light dark force in the galactic center
DOI: 10.1007/JHEP08(2015)050 Bibcode: 2015JHEP...08..050L

Weiner, Neal; Liu, Jia; Xue, Wei

Recent evidence for an excess of gamma rays in the GeV energy range about the Galactic Center have refocused attention on models of dark matter in the low mass regime ( m χ ≲ m Z /2). Because this is an experimentally well-trod energy range, it can be a challenge to develop simple models that explain this excess, consistent…

2015 Journal of High Energy Physics
Planck 68
Helium and multiple populations in the massive globular cluster NGC 6266 (M 62)
DOI: 10.1093/mnras/stu2198 Bibcode: 2015MNRAS.446.1672M

Milone, A. P.

Recent studies suggest that the helium content of multiple stellar populations in globular clusters (GCs) is not uniform. The range of helium varies from cluster to cluster with more massive GCs having, preferentially, large helium spread. GCs with large helium variations also show extended-blue horizontal branch (HB). I exploit Hubble Space Teles…

2015 Monthly Notices of the Royal Astronomical Society
eHST 67
The Spatial Distribution of the Young Stellar Clusters in the Star-forming Galaxy NGC 628
DOI: 10.1088/0004-637X/815/2/93 Bibcode: 2015ApJ...815...93G

Cignoni, M.; Dale, D. A.; Calzetti, D. +21 more

We present a study of the spatial distribution of the stellar cluster populations in the star-forming galaxy NGC 628. Using Hubble Space Telescope broadband WFC3/UVIS UV and optical images from the Treasury Program LEGUS (Legacy ExtraGalactic UV Survey), we have identified 1392 potential young (≲ 100 Myr) stellar clusters within the galaxy using a…

2015 The Astrophysical Journal
eHST 67
Multiwavelength Observations of a Partially Eruptive Filament on 2011 September 8
DOI: 10.1088/0004-637X/805/1/4 Bibcode: 2015ApJ...805....4Z

Feng, L.; Cheng, X.; Guo, Y. +5 more

In this paper, we report our multiwavelength observations of a partial filament eruption event in NOAA active region (AR) 11283 on 8 September 2011. A magnetic null point and the corresponding spine and separatrix surface are found in the AR. Beneath the null point, a sheared arcade supports the filament along the highly complex and fragmented pol…

2015 The Astrophysical Journal
SOHO 67
The High-mass Stellar Initial Mass Function in M31 Clusters
DOI: 10.1088/0004-637X/806/2/198 Bibcode: 2015ApJ...806..198W

Bell, Eric F.; Dolphin, Andrew E.; Skillman, Evan D. +16 more

We have undertaken the largest systematic study of the high-mass stellar initial mass function (IMF) to date using the optical color-magnitude diagrams (CMDs) of 85 resolved, young (4 {Myr}\lt t\lt 25 {Myr}), intermediate mass star clusters (103-104 M), observed as part of the Panchromatic Hubble Andromeda Treasur…

2015 The Astrophysical Journal
eHST 67