Search Publications

Small Polycyclic Aromatic Hydrocarbons in the Red Rectangle
DOI: 10.1086/426498 Bibcode: 2005ApJ...619..368V

Gordon, Karl D.; Witt, Adolf N.; Vijh, Uma P.

Following our initial discovery of blue luminescence in the spectrum of the Red Rectangle (RR) and its identification as fluorescence by small three- to four-ringed polycyclic aromatic hydrocarbon (PAH) molecules, we report on the spatial correlation between the blue luminescence and the 3.3 µm emission, commonly attributed to small, neutral…

2005 The Astrophysical Journal
IUE 51
The X-ray emission from Young Stellar Objects in the ρ Ophiuchi cloud core as seen by XMM-Newton.
DOI: 10.1051/0004-6361:20040480 Bibcode: 2005A&A...429..963O

Grosso, N.; Montmerle, T.; Ozawa, H.

We observed the main core F of the ρ Ophiuchi cloud, an active star-forming region located at d ∼ 140 pc, using XMM-Newton with an exposure of 33 ks. We detect 87 X-ray sources within the 30 arcmin diameter field-of-view of the EPIC imaging detector array. We cross-correlate the positions of XMM-Newton X-ray sources with previous X-ray, infrared (…

2005 Astronomy and Astrophysics
XMM-Newton 51
Inferred acoustic rates of solar p modes from several helioseismic instruments
DOI: 10.1051/0004-6361:20041229 Bibcode: 2005A&A...433..349B

Goupil, M. -J.; Baudin, F.; Chaplin, W. J. +5 more

Acoustic rates of excitation of solar p modes can be estimated from observations in order to place constraints on the modelling of the excitation process and the layers where it occurs in the star. For several reasons (including a poor signal to noise ratio and mode overlap), this estimation is difficult. In this work, we use three completely inde…

2005 Astronomy and Astrophysics
SOHO 51
A Comparison of Absorption- and Emission-Line Abundances in the Nearby Damped Lyα Galaxy SBS 1543+593
DOI: 10.1086/497617 Bibcode: 2005ApJ...635..880B

Bowen, David V.; Tripp, Todd M.; Jenkins, Edward B. +1 more

We have used STIS aboard HST to measure a sulfur abundance of [S/H]=-0.41+/-0.06 in the ISM of the nearby DLA galaxy SBS 1543+593. A direct comparison between this QSO absorption line abundance and abundances measured from H II region emission line diagnostics yields the same result: the abundance of sulfur in the neutral ISM is in good agreement …

2005 The Astrophysical Journal
eHST 51
The Effect of Stellar Evolution on SiC Dust Grain Sizes
DOI: 10.1086/496955 Bibcode: 2005ApJ...634..426S

Speck, Angela K.; Thompson, Grant D.; Hofmeister, Anne M.

Stars on the asymptotic giant branch (AGB) produce dust in their circumstellar shells. The nature of the dust-forming environment is influenced by the evolution of the stars, in terms of both chemistry and density, leading to an evolution in the nature of the dust that is produced. Carbon-rich AGB stars are known to produce silicon carbide (SiC). …

2005 The Astrophysical Journal
ISO 51
A Comparative Study of the Spatial Distribution of Ultraviolet and Far-Infrared Fluxes from M101
DOI: 10.1086/422991 Bibcode: 2005ApJ...619L..75P

Heckman, Timothy M.; Madore, Barry F.; Tuffs, Richard J. +23 more

The total ultraviolet (UV) flux (from 1412 to 2718 Å) of M101 is compared on a pixel-to-pixel basis with the total far-infrared (FIR) flux (from 60 to 170 µm) using the maps of the galaxy taken by the Galaxy Evolution Explorer (GALEX) in the near-UV and far-UV and by the Infrared Space Observatory (ISO) at 60, 100, and 170 µm. The main…

2005 The Astrophysical Journal
ISO 51
Abundances in the H I Envelope of the Extremely Low Metallicity Blue Compact Dwarf Galaxy SBS 0335-052 from Far Ultraviolet Spectroscopic Explorer Observations
DOI: 10.1086/427469 Bibcode: 2005ApJ...621..269T

Thuan, Trinh X.; Izotov, Yuri I.; Lecavelier des Etangs, Alain

We present Far Ultraviolet Spectroscopic Explorer spectroscopy of SBS 0335-052, the second most metal-deficient blue compact dwarf (BCD) galaxy known [log(O/H)=-4.70]. In addition to the H I Lyman series, we detect C II, N I, N II, O I, Si II, Ar I, and Fe II absorption lines, mainly arising from the extended H I envelope in which SBS 0335-052 is …

2005 The Astrophysical Journal
eHST 51
Localized fast flow disturbance observed in the plasma sheet and in the ionosphere
DOI: 10.5194/angeo-23-553-2005 Bibcode: 2005AnGeo..23..553N

Balogh, A.; Lester, M.; André, M. +8 more

An isolated plasma sheet flow burst took place at 22:02 UT, 1 September 2002, when the Cluster footpoint was located within the area covered by the Magnetometers-Ionospheric Radars-All-sky Cameras Large Experiment (MIRACLE). The event was associated with a clear but weak ionospheric disturbance and took place during a steady southward IMF interval…

2005 Annales Geophysicae
Cluster 50
Oxygen Ions Observed Near Saturn's A Ring
DOI: 10.1126/science.1105734 Bibcode: 2005Sci...307.1260W

Luhmann, J. G.; Ip, W. -H.; Mueller-Wodarg, I. +8 more

Ions were detected in the vicinity of Saturn's A ring by the Ion and Neutral Mass Spectrometer (INMS) instrument onboard the Cassini Orbiter during the spacecraft's passage over the rings. The INMS saw signatures of molecular and atomic oxygen ions and of protons, thus demonstrating the existence of an ionosphere associated with the A ring. A like…

2005 Science
Cassini 50
New Silhouette Disks with Reflection Nebulae and Outflows in the Orion Nebula and M43
DOI: 10.1086/426567 Bibcode: 2005AJ....129..382S

Smith, Nathan; Bally, John; Walawender, Josh +1 more

We report the detection of several new circumstellar disks seen in silhouette against background nebular light in the outskirts of the Orion Nebula and the neighboring H II region M43. These were detected as part of our Hα survey of Orion with the Advanced Camera for Surveys on board the Hubble Space Telescope. Several of the disks show bipolar re…

2005 The Astronomical Journal
eHST 50