Search Publications

Velocity resolved [C ii], [C i], and CO observations of the N159 star-forming region in the Large Magellanic Cloud: a complex velocity structure and variation of the column densities
DOI: 10.1051/0004-6361/201525630 Bibcode: 2015A&A...580A..54O

Wiesemeyer, Helmut; Güsten, Rolf; Okada, Yoko +4 more

Context. The [C ii] 158 µm fine structure line is one of the dominant cooling lines in star-forming active regions. Together with models of photon-dominated regions, the data is used to constrain the physical properties of the emitting regions, such as the density and the radiation field strength. According to the modeling, the [C ii] 158 &m…

2015 Astronomy and Astrophysics
Herschel 27
The Flare-ona of EK Draconis
DOI: 10.1088/0004-6256/150/1/7 Bibcode: 2015AJ....150....7A

Ayres, Thomas R.

EK Draconis (HD 129333: G1.5 V) is a well-known young (50 Myr) solar analog. In 2012, Hubble Space Telescope returned to EK Dra to follow up a far-ultraviolet (FUV) SNAPshot visit by Cosmic Origins Spectrograph (COS) two years earlier. The brief SNAP pointing had found surprisingly redshifted, impulsively variable subcoronal “hot-line” emission of…

2015 The Astronomical Journal
eHST 27
The growth index of matter perturbations using the clustering of dark energy
DOI: 10.1093/mnras/stv411 Bibcode: 2015MNRAS.449.2151B

Basilakos, Spyros

We have put forward a new unified framework which provides a consistent and rather complete account of the growth index of matter perturbations in the regime where the dark energy is allowed to have clustering. In particular, we find that the growth index is not only affected by the cosmological parameters but rather it depends on the choice of th…

2015 Monthly Notices of the Royal Astronomical Society
Planck 27
Radio Timing and Optical Photometry of the Black Widow System PSR J1953+1846A in the Globular Cluster M71
DOI: 10.1088/0004-637X/807/1/91 Bibcode: 2015ApJ...807...91C

Dalessandro, E.; Ransom, S. M.; Ferraro, F. R. +6 more

We report on the determination of the astrometric, spin, and orbital parameters for PSR J1953+1846 A, a “black widow” binary millisecond pulsar in the globular cluster M71. By using the accurate position and orbital parameters obtained from radio timing, we identified the optical companion in Advanced Camera for Surveys/Hubble Space Telescope imag…

2015 The Astrophysical Journal
eHST 27
Observations and Modeling of North-South Asymmetries Using a Flux Transport Dynamo
DOI: 10.1088/0004-637X/799/2/220 Bibcode: 2015ApJ...799..220S

Tripathi, Durgesh; Shetye, Juie; Dikpati, Mausumi

The peculiar behavior of solar cycle 23 and its prolonged minima has been one of the most studied problems over the past few years. In the present paper, we study the asymmetries in active region magnetic flux in the northern and southern hemispheres during the complete solar cycle 23 and the rising phase of solar cycle 24. During the declining ph…

2015 The Astrophysical Journal
SOHO 27
Mars thermospheric scale height: CO Cameron and CO2+ dayglow observations from Mars Express
DOI: 10.1016/j.icarus.2014.09.051 Bibcode: 2015Icar..245..295S

Montmessin, F.; Bertaux, J. -L.; Gérard, J. -C. +3 more

The CO Cameron (170-270 nm) and CO2+ ultraviolet doublet (298 and 299 nm) emissions have been observed on the Mars dayside with Mars Express Spectroscopy for Investigation of Characteristics of the Atmosphere of Mars (SPICAM) instrument in the limb viewing mode. These ultraviolet emissions ultimately arise from the excitation…

2015 Icarus
MEx 27
Multiscale study of electron energization during unsteady reconnection events
DOI: 10.1002/2014JA020316 Bibcode: 2015JGRA..120.4784A

Lapenta, Giovanni; El-Alaoui, Mostafa; Walker, Raymond J. +2 more

Understanding particle acceleration in the magnetotail during substorms requires knowledge of changes in the global magnetospheric configuration and the local regions of intense fields and microinstabilities caused by processes associated with reconnection. We simulated a substorm on 15 February 2008 by coupling the University of California, Los A…

2015 Journal of Geophysical Research (Space Physics)
Cluster 27
Co-spatial Long-slit UV/Optical AL Spectra of 10 Galactic Planetary Nebulae with HST/STIS. I. Description of the Observations, Global Emission-line Measurements, and CNO Abundances
DOI: 10.1088/0004-637X/803/1/23 Bibcode: 2015ApJ...803...23D

Corradi, Romano L. M.; Balick, Bruce; Shaw, Richard A. +3 more

We present observations and initial analysis from a Hubble Space Telescope (HST) Cycle 19 program using STIS to obtain the first co-spatial, UV-optical spectra of 10 Galactic planetary nebulae (PNs). Our primary objective was to measure the critical emission lines of carbon and nitrogen with unprecedented signal-to-noise ratio (S/N) and spatial re…

2015 The Astrophysical Journal
eHST 27
Chemical Abundances and Properties of the Ionized Gas in NGC 1705
DOI: 10.1088/0004-6256/150/5/143 Bibcode: 2015AJ....150..143A

Tosi, M.; Mignoli, M.; Aloisi, A. +3 more

We obtained [O iii] narrow-band imaging and multi-slit MXU spectroscopy of the blue compact dwarf (BCD) galaxy NGC 1705 with FORS2@VLT to derive chemical abundances of planetary nebulae and H ii regions and, more in general, to characterize the properties of the ionized gas. The auroral [O iii]λ 4363 line was detected in all but 1 of the 11 analyz…

2015 The Astronomical Journal
eHST 27
Relativistic electron acceleration during HILDCAA events: are precursor CIR magnetic storms important?
DOI: 10.1186/s40623-015-0280-5 Bibcode: 2015EP&S...67..109H

Hajra, Rajkumar; Tsurutani, Bruce T.; Gonzalez, Walter D. +4 more

We present a comparative study of high-intensity long-duration continuous AE activity (HILDCAA) events, both isolated and those occurring in the "recovery phase" of geomagnetic storms induced by corotating interaction regions (CIRs). The aim of this study is to determine the difference, if any, in relativistic electron acceleration and magnetosphe…

2015 Earth, Planets and Space
Cluster 27