Search Publications

EMIC triggered chorus emissions in Cluster data
DOI: 10.1002/jgra.50178 Bibcode: 2013JGRA..118.1159G

Pickett, J. S.; SantolíK, O.; Cornilleau-Wehrlin, N. +6 more

Electromagnetic ion cyclotron (EMIC) triggered chorus emissions have recently been a subject of several experimental, theoretical and simulation case studies, noting their similarities with whistler-mode chorus. We perform a survey of 8 years of Cluster data in order to increase the database of EMIC triggered emissions. The results of this is that…

2013 Journal of Geophysical Research (Space Physics)
Cluster 37
Solar Magnetic Tracking. IV. The Death of Magnetic Features
DOI: 10.1088/0004-637X/774/2/127 Bibcode: 2013ApJ...774..127L

Lamb, D. A.; DeForest, C. E.; Parnell, C. E. +2 more

The removal of magnetic flux from the quiet-Sun photosphere is important for maintaining the statistical steady state of the magnetic field there, for determining the magnetic flux budget of the Sun, and for estimating the rate of energy injected into the upper solar atmosphere. Magnetic feature death is a measurable proxy for the removal of detec…

2013 The Astrophysical Journal
Hinode 36
Kinematics of the Intermediate-mass Black Hole Candidate HLX-1
DOI: 10.1088/2041-8205/768/1/L22 Bibcode: 2013ApJ...768L..22S

Soria, Roberto; Hau, George K. T.; Pakull, Manfred W.

We studied the optical spectrum of HLX-1 during its latest outburst, using the FORS2 spectrograph on the Very Large Telescope. We detect an Hα emission line centered at λ = 6718.9 ± 0.9 Å and find that its projected radial velocity with respect to the nucleus of ESO 243-49 is 424 ± 27 km s-1, while the maximum rotational velocity of the…

2013 The Astrophysical Journal
eHST 36
Giant Lobes of Centaurus A Radio Galaxy Observed with the Suzaku X-Ray Satellite
DOI: 10.1088/0004-637X/766/1/48 Bibcode: 2013ApJ...766...48S

Simionescu, A.; Cheung, C. C.; Fukazawa, Y. +15 more

We report on Suzaku observations of selected regions within the southern giant lobe of the radio galaxy Centaurus A. In our analysis we focus on distinct X-ray features detected with the X-ray Imaging Spectrometer within the range 0.5-10 keV, some of which are likely associated with fine structure of the lobe revealed by recent high-quality radio …

2013 The Astrophysical Journal
Suzaku 36
The ACS LCID Project - VIII. The short-period Cepheids of Leo A
DOI: 10.1093/mnras/stt655 Bibcode: 2013MNRAS.432.3047B

Skillman, Evan D.; Cole, Andrew A.; Tolstoy, Eline +9 more

We present the results of a new search for variable stars in the Local Group dwarf galaxy Leo A, based on deep photometry from the Advanced Camera for Surveys onboard the Hubble Space Telescope. We detected 166 bona fide variables in our field, of which about 60 per cent are new discoveries and 33 candidate variables. Of the confirmed variables, w…

2013 Monthly Notices of the Royal Astronomical Society
eHST 36
Azimuthal directions of equatorial noise propagation determined using 10 years of data from the Cluster spacecraft
DOI: 10.1002/2013JA019373 Bibcode: 2013JGRA..118.7160N

Pickett, J. S.; Santolík, O.; Němec, F. +2 more

Equatorial noise (EN) emissions are electromagnetic waves at frequencies between the proton cyclotron frequency and the lower hybrid frequency routinely observed within a few degrees of the geomagnetic equator at radial distances from about 2 to 6 RE. They propagate in the extraordinary (fast magnetosonic) mode nearly perpendicularly to…

2013 Journal of Geophysical Research (Space Physics)
Cluster 36
Fine-structure Fe II* Emission and Resonant Mg II Emission in z ~ 1 Star-forming Galaxies
DOI: 10.1088/0004-637X/774/1/50 Bibcode: 2013ApJ...774...50K

Weiner, Benjamin J.; Martin, Crystal L.; Shapley, Alice E. +3 more

We present a study of the prevalence, strength, and kinematics of ultraviolet Fe II and Mg II emission lines in 212 star-forming galaxies at z ~ 1 selected from the DEEP2 survey. We find Fe II* emission in composite spectra assembled on the basis of different galaxy properties, indicating that Fe II* emission is common at z ~ 1. In these composite…

2013 The Astrophysical Journal
eHST 36
HST/COS observations of a new population of associated QSO absorbers
DOI: 10.1093/mnras/stt390 Bibcode: 2013MNRAS.431.2885M

Savage, B. D.; Narayanan, A.; Arav, N. +2 more

We present a sample of new population of associated absorbers, detected through Ne VIII λλ770, 780 absorption, in the Hubble Space Telescope (HST)/Cosmic Origins Spectrograph (COS) spectra of intermediate-redshift (0.45 < z < 1.21) quasars (QSOs). Our sample comprised of total 12 associated Ne VIII systems detected towards eight lines of sig…

2013 Monthly Notices of the Royal Astronomical Society
eHST 36
Evidence of quasi-chemically homogeneous evolution of massive stars up to solar metallicity
DOI: 10.1051/0004-6361/201321282 Bibcode: 2013A&A...554A..23M

Martins, F.; Mahy, L.; Russeil, D. +1 more

Context. Long soft gamma-ray bursts (LGRBs) are usually associated with the death of the most massive stars. A large amount of core angular momentum in the phases preceding the explosion is required to form LGRBs. A very high initial rotational velocity can provide this angular momentum. This velocity strongly influences the way the star evolves: …

2013 Astronomy and Astrophysics
IUE 36
Saturn's cloud structure inferred from Cassini ISS
DOI: 10.1016/j.icarus.2013.03.015 Bibcode: 2013Icar..225...93R

Roman, Michael T.; Gierasch, Peter J.; Banfield, Don

Using high-resolution Cassini ISS images with wavelengths ranging from the ultraviolet to the near infrared, we have retrieved Saturn's atmospheric aerosol structure and properties for a broad range of latitudes in the southern hemisphere. The observations are consistent with two distinct layers of haze above a scattered cloud. Each layer is chara…

2013 Icarus
Cassini 36