Search Publications

Discovery of Bright Galactic R Coronae Borealis and DY Persei Variables: Rare Gems Mined from ACVS
DOI: 10.1088/0004-637X/755/2/98 Bibcode: 2012ApJ...755...98M

Cenko, S. B.; Bloom, J. S.; Stassun, K. G. +4 more

We present the results of a machine-learning (ML)-based search for new R Coronae Borealis (RCB) stars and DY Persei-like stars (DYPers) in the Galaxy using cataloged light curves from the All-Sky Automated Survey (ASAS) Catalog of Variable Stars (ACVS). RCB stars—a rare class of hydrogen-deficient carbon-rich supergiants—are of great interest owin…

2012 The Astrophysical Journal
AKARI 19
Solar-Storm/Lunar Atmosphere Model (SSLAM): An overview of the effort and description of the driving storm environment
DOI: 10.1029/2012JE004070 Bibcode: 2012JGRE..117.0K04F

Delory, G. T.; Halekas, J. S.; Farrell, W. M. +9 more

On 29 April 1998, a coronal mass ejection (CME) was emitted from the Sun that had a significant impact at Earth. The terrestrial magnetosphere became more electrically active during the storm passage. Less explored is the effect of such a storm on an exposed rocky body like our Moon. The solar-storm/lunar atmosphere modeling effort (SSLAM) brings …

2012 Journal of Geophysical Research (Planets)
SOHO 19
Star-galaxy separation in the AKARI NEP deep field
DOI: 10.1051/0004-6361/201118108 Bibcode: 2012A&A...541A..50S

Pearson, C. P.; Ohyama, Y.; Takagi, T. +10 more

Context. It is crucial to develop a method for classifying objects detected in deep surveys at infrared wavelengths. We specifically need a method to separate galaxies from stars using only the infrared information to study the properties of galaxies, e.g., to estimate the angular correlation function, without introducing any additional bias.

2012 Astronomy and Astrophysics
AKARI 19
Magnetic field measurements during the ROSETTA flyby at asteroid (21)Lutetia
DOI: 10.1016/j.pss.2011.08.009 Bibcode: 2012P&SS...66..155R

Richter, I.; Glassmeier, K. H.; Carr, C. M. +5 more

On July 10, 2010, the ROSETTA spacecraft performed a flyby at asteroid (21)Lutetia at a solar distance of 2.72 AU. The spacecraft-asteroid distance at closest approach was 3120 km. The magnetometers onboard ROSETTA were operating but did not detect any conclusive signature of the asteroid. Any magnetic field signature which could possibly be attri…

2012 Planetary and Space Science
Rosetta 19
AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: Mid-infrared View of Transition Galaxies
DOI: 10.1088/0004-637X/745/2/181 Bibcode: 2012ApJ...745..181K

Kim, Seong Jin; Papovich, Casey; Weiner, Benjamin J. +12 more

We present the mid-infrared (MIR) properties of galaxies within a supercluster in the north ecliptic pole region at z ~ 0.087 observed with the AKARI satellite. We use data from the AKARI NEP-Wide (5.4 deg2) IR survey and the CLusters of galaxies EVoLution studies (CLEVL) mission program. We show that near-IR (3 µm)-mid-IR (11 &mi…

2012 The Astrophysical Journal
AKARI 19
Water in star- and planet-forming regions
DOI: 10.1098/rsta.2011.0301 Bibcode: 2012RSPTA.370.2778B

van Dishoeck, E. F.; Bergin, E. A.

In this paper we discuss the astronomical search for water vapor in order to understand the disposition of water in all its phases throughout the process of star and planet formation. Our ability to detect and study water vapor has recently received a tremendous boost with the successful launch and operations of the Herschel Space Observatory. Her…

2012 Philosophical Transactions of the Royal Society of London Series A
Herschel 19
The blue straggler star population in NGC 6229
DOI: 10.1111/j.1365-2966.2012.20690.x Bibcode: 2012MNRAS.422.1171S

Dalessandro, E.; Sanna, N.; Beccari, G. +3 more

We have used a combination of high-resolution Hubble Space Telescope Wide Field Planetary Camera 2 and wide-field ground-based observations in ultraviolet and optical bands to study the blue straggler star (BSS) population of the outer halo globular cluster NGC 6229 over its entire radial extent. A total of 64 bright BSS (with m255≤ 21.…

2012 Monthly Notices of the Royal Astronomical Society
eHST 19
Three quasi-stellar objects acting as strong gravitational lenses
DOI: 10.1051/0004-6361/201118015 Bibcode: 2012A&A...540A..36C

Djorgovski, S. G.; Stern, D.; Faure, C. +8 more

We report the discovery of three new cases of quasi-stellar objects (QSOs) acting as strong gravitational lenses on background emission line galaxies: SDSS J0827+5224 (zQSO = 0.293, zs = 0.412), SDSS J0919+2720 (zQSO = 0.209, zs = 0.558), SDSS J1005+4016 (zQSO = 0.230, zs = 0.441). …

2012 Astronomy and Astrophysics
eHST 19
Changes in the magnetotail configuration before near-Earth reconnection
DOI: 10.1029/2011JA017040 Bibcode: 2012JGRA..117.2219S

Gordeev, E. I.; Snekvik, K.; Østgaard, N. +4 more

We have examined three typical substorm growth phase signatures in the magnetotail two hours before near Earth reconnection; namely current sheet thinning, field line stretching and increase in the lobe magnetic pressure. The reconnection events were identified from in situ measurements in the plasma sheet by the Cluster spacecraft. The events wer…

2012 Journal of Geophysical Research (Space Physics)
Cluster 19
2M1155-79 (= T Chamaeleontis B): A Low-mass, Wide-separation Companion to the nearby, "Old" T Tauri Star T Chamaeleontis
DOI: 10.1088/2041-8205/747/2/L23 Bibcode: 2012ApJ...747L..23K

Montez, Rodolfo; Murphy, Simon J.; Kastner, Joel H. +3 more

The early-K star T Cha, a member of the nearby (D ≈ 100 pc) epsilon Cha Association, is a relatively "old" (age ~ 7 Myr) T Tauri star that is still sporadically accreting from an orbiting disk whose inner regions are now evidently being cleared by a close, substellar companion. We report the identification, via analysis of proper motions, serendip…

2012 The Astrophysical Journal
XMM-Newton 19