Search Publications

Deep near-infrared adaptive-optics observations of a young embedded cluster at the edge of the RCW 41 H II region
DOI: 10.1051/0004-6361/201425464 Bibcode: 2015A&A...576A.110N

Zavagno, A.; Neichel, B.; Samal, M. R. +3 more


Aims: We investigate the star formation activity in a young star forming cluster embedded at the edge of the RCW 41 H ii region. As a complementary goal, we aim to demonstrate the gain provided by wide-field adaptive optics (WFAO) instruments to study young clusters.
Methods: We used deep, JHKs images from the newly commission…

2015 Astronomy and Astrophysics
eHST 15
Investigation of the RCR catalog sources in the millimeter and submillimeter ranges based on the Planck mission data
DOI: 10.1134/S1990341315020030 Bibcode: 2015AstBu..70..156V

Verkhodanov, O. V.; Majorova, E. K.; Zhelenkova, O. P. +3 more

We have studied the regions of the microwave background radiation maps of the Planck experiment in the neighborhood of the RCR catalog radio sources. From the processed data for bright radio sources in the microwave range, we plotted the calibration curves which allow the brightness of the objects to be measured. For the first time, for 117 object…

2015 Astrophysical Bulletin
Planck 15
The Chandra/HETG view of NGC 1365 in a Compton-thick state
DOI: 10.1093/mnras/stv1826 Bibcode: 2015MNRAS.453.2558N

Reeves, J. N.; Braito, V.; Gofford, J. +3 more

We present the analysis of a Chandra High-Energy Transmission Grating (HETG) observation of the local Seyfert galaxy NGC 1365. The source, well known for its dramatic X-ray spectral variability, was caught in a reflection-dominated, Compton-thick state. The high spatial resolution afforded by Chandra allowed us to isolate the soft X-ray emission f…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 15
Temperatures of dust and gas in S 140
DOI: 10.1051/0004-6361/201525669 Bibcode: 2015A&A...580A..68K

Ossenkopf, V.; van der Tak, F. F. S.; Kramer, C. +4 more

Context. In dense parts of interstellar clouds (≥105 cm-3), dust and gas are expected to be in thermal equilibrium, being coupled via collisions. However, previous studies have shown that in the presence of intense radiation fields, the temperatures of the dust and gas may remain decoupled even at higher densities.
Aims:…

2015 Astronomy and Astrophysics
Herschel 15
First extreme and far ultraviolet spectrum of a Comet Nucleus: Results from 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2015.04.023 Bibcode: 2015Icar..256..117S

Stern, S. A.; Feldman, P. D.; Bertaux, J. -L. +7 more

We used the Alice spectrograph onboard the Rosetta comet orbiter spacecraft to observe the surface of Comet 67P/Churyumov-Gerasimenko in the extreme and far ultraviolet (EUV/FUV) from 700 to 2050 Å in mid-August 2014. These observations were before significant EUV/FUV coma signatures were observed by Alice. The resulting coadded spectrum has high …

2015 Icarus
Rosetta 15
Uncovering the Nucleus Candidate for NGC 253
DOI: 10.1088/0004-6256/150/5/139 Bibcode: 2015AJ....150..139G

Schirmer, M.; Díaz, R. J.; Günthardt, G. I. +4 more

NGC 253 is the nearest spiral galaxy with a nuclear starburst that becomes the best candidate for studying the relationship between starburst and active galactic nucleus activity. However, this central region is veiled by large amounts of dust, and it has been so far unclear which is the true dynamical nucleus to the point that there is no strong …

2015 The Astronomical Journal
eHST 15
Dynamics of Microwave Sources Associated with the Neutral Line and the Magnetic-Field Parameters of Sunspots as a Factor in Predicting Large Flares
DOI: 10.1007/s11207-014-0605-8 Bibcode: 2015SoPh..290...53A

Abramov-Maximov, V. E.; Borovik, V. N.; Opeikina, L. V. +1 more

We studied the evolution of five active regions (ARs) where strong X-class flares occurred in 2011 - 2012 (NOAA ARs 11158, 11166, 11263, 11283 and 11520). Our study focuses on the pre-flare phase of these ARs (during a few days before the flare) to reveal features in the microwave radiation and magnetic-field characteristics of the ARs that indica…

2015 Solar Physics
SOHO 15
The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models' X-Ray Emission
DOI: 10.1088/0004-637X/800/2/102 Bibcode: 2015ApJ...800..102H

Henley, David B.; Shelton, Robin L.; Hill, Alex S. +2 more

We test the X-ray emission predictions of galactic fountain models against XMM-Newton measurements of the emission from the Milky Way's hot halo. These measurements are from 110 sight lines, spanning the full range of Galactic longitudes. We find that a magnetohydrodynamical simulation of a supernova-driven interstellar medium, which features a fl…

2015 The Astrophysical Journal
XMM-Newton 15
Cross-correlation of Near- and Far-infrared Background Anisotropies as Traced by Spitzer and Herschel
DOI: 10.1088/0004-637X/811/2/125 Bibcode: 2015ApJ...811..125T

Gong, Yan; Cooray, Asantha; Mitchell-Wynne, Ketron +3 more

We present the cross-correlation between the far-infrared (far-IR) background fluctuations as measured with the Herschel Space Observatory at 250, 350, and 500 µm and the near-infrared (near-IR) background fluctuations with the Spitzer Space Telescope at 3.6 and 4.5 µm. The cross-correlation between the FIR and NIR background anisotrop…

2015 The Astrophysical Journal
Herschel 15
Transpolar arc observation after solar wind entry into the high-latitude magnetosphere
DOI: 10.1002/2014JA020912 Bibcode: 2015JGRA..120.3525M

Wei, Y.; Zong, Q. -G.; Fear, R. C. +11 more

Recently, Cluster observations have revealed the presence of new regions of solar wind plasma entry at the high-latitude magnetospheric lobes tailward of the cusp region, mostly during periods of northward interplanetary magnetic field. In this study, observations from the Global Ultraviolet Imager (GUVI) experiment on board the TIMED spacecraft a…

2015 Journal of Geophysical Research (Space Physics)
Cluster 15