Search Publications

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
A Simultaneous Forbush Decrease Associated with an Earthward Coronal Mass Ejection Observed by STEREO
DOI: 10.1007/s11207-012-0053-2 Bibcode: 2012SoPh..280..197O

Yi, Y.; Oh, S. Y.

The intensity-time profile of Forbush decrease (FD) events observed by neutron monitors (NMs) looks like that of a geomagnetic storm as defined by the Dst index. Oh, Yi, and Kim (J. Geophys. Res. 113, A01103, 2008) and Oh and Yi (J. Geophys. Res. 114, A11102, 2009) classified FD events based on the amount of overlap and simultaneity of their main …

2012 Solar Physics
SOHO 19
Evidence for Fresh Frost Layer on the Bare Nucleus of Comet Hale-Bopp at 32 AU Distance
DOI: 10.1088/0004-637X/761/1/8 Bibcode: 2012ApJ...761....8S

Pál, András; Sárneczky, Krisztián; Juhász, Attila +4 more

Here, we report that the activity of comet Hale-Bopp ceased between late 2007 and 2009 March, at about 28 AU distance from the Sun. At that time, the comet resided at a distance from the Sun that exceeded the freeze-out distance of regular comets by an order of magnitude. A Herschel Space Observatory PACS scan was taken in mid-2010, in the already…

2012 The Astrophysical Journal
Herschel eHST 19
Herschel and JCMT observations of the early-type dwarf galaxy NGC 205
DOI: 10.1111/j.1365-2966.2012.21044.x Bibcode: 2012MNRAS.423.2359D

Boquien, M.; Roussel, H.; Fritz, J. +18 more

We present Herschel dust continuum, James Clerk Maxwell Telescope CO (3-2) observations and a search for [C II] 158 ?m and [O I] 63 ?m spectral line emission for the brightest early-type dwarf satellite of Andromeda, NGC 205. While direct gas measurements [Mg∼ 1.5 × 106 M, H I+ CO (1-0)] have proven to be inconsis…

2012 Monthly Notices of the Royal Astronomical Society
Herschel 19
The XMM-Newton survey of the Small Magellanic Cloud: XMMU J010633.1-731543 and XMMU J010743.1-715953, two new Be/X-ray binary systems
DOI: 10.1111/j.1365-2966.2012.21193.x Bibcode: 2012MNRAS.424..282C

Haberl, F.; Hatzidimitriou, D.; Mereghetti, S. +6 more

In the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), two new bright X-ray sources were discovered exhibiting the spectral characteristics of high-mass X-ray binaries - but revealing only weak evidence for pulsations in just one of the objects (at 153 s in XMMU J010743.1-715953). The accurate X-ray source locations permit the…

2012 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
Ultraviolet Measurements of Interstellar C2
DOI: 10.1088/0004-637X/761/1/38 Bibcode: 2012ApJ...761...38H

Federman, S. R.; Sheffer, Y.; Hupe, Ryan C.

We analyzed archival spectra acquired with the Hubble Space Telescope for a study of interstellar C2. Absorption from the electronic transitions, D 1Σ+ u - X 1Σ+ g (0,0) as well as F 1Πu - X 1Σ+ g (0,0) and (1,0), was…

2012 The Astrophysical Journal
eHST 19