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From CoRoT 102899501 to the Sun. A time evolution model of chromospheric activity on the main sequence
DOI: 10.1051/0004-6361/201219101 Bibcode: 2012A&A...548A..15G

Deleuil, M.; Fridlund, M.; Gondoin, P. +7 more


Aims: The present study reports measurements of the rotation period of a young solar analogue, estimates of its surface coverage by photospheric starspots and of its chromospheric activity level, and derivations of its evolutionary status. Detailed observations of many young solar-type stars, such as the one reported in the present paper, pro…

2012 Astronomy and Astrophysics
CoRoT 12
A Rare Early-type Star Revealed in the Wing of the Small Magellanic Cloud
DOI: 10.1088/0004-637X/753/2/173 Bibcode: 2012ApJ...753..173E

Gruendl, R. A.; Hamann, W. -R.; Gallagher, J. S., III +6 more

Sk 183 is the visually brightest star in the N90 nebula, a young star-forming region in the Wing of the Small Magellanic Cloud (SMC). We present new optical spectroscopy from the Very Large Telescope which reveals Sk 183 to be one of the most massive O-type stars in the SMC. Classified as an O3-type dwarf on the basis of its nitrogen spectrum, the…

2012 The Astrophysical Journal
IUE eHST 12
CO Structure of the 21 µm Source IRAS 22272+5435: A Sign of a Jet Launch?
DOI: 10.1088/0004-637X/759/1/61 Bibcode: 2012ApJ...759...61N

Zhang, Yong; Kwok, Sun; Yung, Bosco H. K. +3 more

We report the results of radio interferometric observations of the 21 µm source IRAS 22272+5435 in the CO J = 2-1 line. 21 µm sources are carbon-rich objects in the post-asymptotic-giant-branch phase of evolution, which show an unidentified emission feature at 21 µm. Since 21 µm sources usually also have circumstellar molec…

2012 The Astrophysical Journal
eHST 12
X-Ray and Near-infrared Observations of the Obscured Accreting Pulsar IGR J18179-1621
DOI: 10.1088/0004-637X/757/2/143 Bibcode: 2012ApJ...757..143N

Nowak, M. A.; Chaty, S.; Rodriguez, J. +6 more

IGR J18179-1621 is an obscured accreting X-ray pulsar discovered by INTEGRAL on 2012 February 29. We report on our 20 ks Chandra-High Energy Transmission Gratings Spectrometer observation of the source performed on 2012 March 17, on two short contemporaneous Swift observations, and on our two near-infrared (Ks , Hn , and J

2012 The Astrophysical Journal
INTEGRAL 12
Determining the North-South Displacement of the Heliospheric Current Sheet from Coronal Streamer Observations
DOI: 10.1088/0004-637X/755/2/135 Bibcode: 2012ApJ...755..135R

Wang, Y. -M.; Robbrecht, E.

Inferences based on interplanetary field measurements have suggested a statistical tendency for the heliospheric current sheet (HCS) to be displaced southward of the heliographic equator during the past four solar cycles. Here, we use synoptic maps of white-light streamer structures to determine more directly the longitudinally averaged latitude o…

2012 The Astrophysical Journal
SOHO 12
Extreme-ultraviolet Spectroscopic Observation of Direct Coronal Heating during a C-class Solar Flare
DOI: 10.1088/0004-637X/754/1/54 Bibcode: 2012ApJ...754...54B

Brosius, Jeffrey W.

With the Coronal Diagnostic Spectrometer operating in rapid cadence (9.8 s) stare mode during a C6.6 flare on the solar disk, we observed a sudden brightening of Fe XIX line emission (formed at temperature T ≈ 8 MK) above the pre-flare noise without a corresponding brightening of emission from ions formed at lower temperatures, including He I (0.0…

2012 The Astrophysical Journal
SOHO 12
Empirical near-infrared colors for low-mass stars and brown dwarfs in the Orion Nebula Cluster. An empirical near-infrared isochrone at ~1 Myr
DOI: 10.1051/0004-6361/201219264 Bibcode: 2012A&A...545A..19S

Robberto, M.; Scandariato, G.; Da Rio, N. +2 more

Context. Current atmospheric and evolutionary models for low-mass stars and brown dwarfs rely on approximate assumptions on the physics of the stellar structure and the atmospheric radiative transfer. This leads to biased theoretical predictions on the photospheric spectral energy distributions of these system, especially when applied to low surfa…

2012 Astronomy and Astrophysics
eHST 12
Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters
DOI: 10.1088/0004-637X/760/1/65 Bibcode: 2012ApJ...760...65F

Hsia, Chih-Hao; Yung, Bosco H. K.; Nakashima, Jun-ichi +2 more

We report the results of Australia Telescope Compact Array observations of the Westerlund 1 (Wd1) region in the SiO v = 1, J = 1-0, and H2O 616-523 maser lines, and we also report the analysis of maser properties of red supergiants (RSGs) associated with six massive clusters including Wd1. The primary purpose of th…

2012 The Astrophysical Journal
AKARI 12
Abrupt Changes of the Photospheric Magnetic Field in Active Regions and the Impulsive Phase of Solar Flares
DOI: 10.1088/0004-637X/756/2/144 Bibcode: 2012ApJ...756..144C

Petrie, G. J. D.; Ling, A. G.; Cliver, E. W.

We compared time profiles of changes of the unsigned photospheric magnetic flux in active regions with those of their associated soft X-ray (SXR) bursts for a sample of 75 >= M5 flares well observed by Global Oscillation Network Group longitudinal magnetographs. Sixty-six of these events had stepwise changes in the spatially integrated unsigned…

2012 The Astrophysical Journal
SOHO 12
The electromagnetic pickup of submicron-sized dust above Enceladus's northern hemisphere
DOI: 10.1016/j.icarus.2012.02.033 Bibcode: 2012Icar..219..498F

Gurnett, Donald A.; Farrell, William M.; Kurth, William S. +3 more

As the saturnian magnetoplasma sweeps past Enceladus, it experiences both a decrease in electron content and sharp slowdown in the northern hemisphere region within ∼5 Enceladus Radii (Re). This slowdown is observed by Cassini in regions not obviously associated with the southern directed plume-originating ions. We suggest herein that t…

2012 Icarus
Cassini 12