Search Publications

Ultraviolet-Optical Pixel Maps of Face-on Spiral Galaxies: Clues for Dynamics and Star Formation Histories
DOI: 10.1086/367820 Bibcode: 2003ApJ...586..923E

Conselice, Christopher J.; de Grijs, Richard; Windhorst, Rogier A. +8 more

Ultraviolet and optical images of the face-on spiral galaxies NGC 6753 and NGC 6782 reveal regions of strong ongoing star formation that are associated with structures traced by the old stellar populations. We use these images to construct NUV-(NUV-I814) pixel color-magnitude diagrams (pCMDs) that reveal plumes of pixels with strongly v…

2003 The Astrophysical Journal
eHST 18
The Gravitational Lens B1608+656. I. V-, I-, and H-Band Hubble Space Telescope Imaging
DOI: 10.1086/345592 Bibcode: 2003ApJ...584..100S

Blandford, R. D.; Surpi, G.

We present a multiwavelength analysis of high-resolution observations of the quadruple lens B1608+656 from the Hubble Space Telescope archive, acquired with WFPC2 through filters F606W (V band) and F814W (I band) and with NIC1 in filter F160W (H band). In the three bands, the observations show extended emission from the four images of the source i…

2003 The Astrophysical Journal
eHST 18
The Quintuple Quasar: Radio and Optical Observations
DOI: 10.1086/374832 Bibcode: 2003ApJ...590...26W

Keeton, Charles R.; Winn, Joshua N.; Kochanek, Christopher S. +1 more

We present results from high-resolution radio and optical observations of PMN J0134-0931, a gravitational lens with a unique radio morphology and an extremely red optical counterpart. Our data support the theory of Keeton & Winn: five of the six observed radio components are multiple images of a single quasar, produced by a pair of lens galaxi…

2003 The Astrophysical Journal
eHST 18
Hα Impact Polarization Observed in a Gradual Flare
DOI: 10.1086/378123 Bibcode: 2003ApJ...596.1347H

Hanaoka, Y.

Linear polarization of the Hα line was detected in kernels of a gradual flare, which was accompanied by a filament eruption. The maximum degree of polarization of this flare exceeds 1%, and the orientation of the polarization is approximately perpendicular to the flare ribbons. These results can be explained with the assumption that the observed p…

2003 The Astrophysical Journal
SOHO 18
Hubble Space Telescope STIS Spectroscopy of the White Dwarfs in the Ultrashort-Period Dwarf Novae VY Aquarii and WX Ceti
DOI: 10.1086/345445 Bibcode: 2003ApJ...583..907S

Szkody, Paula; Howell, Steve B.; Sion, Edward M. +2 more

We present the results of a multicomponent synthetic spectral analysis of Hubble Space Telescope (HST) STIS spectra of the ultrashort-period dwarf novae VY Aqr and WX Ceti during their deep quiescence following their last superoutburst. The white dwarf in these extremely low accretion rate systems dominates the far-UV light. We find that the accre…

2003 The Astrophysical Journal
eHST 18
Spectroscopic Identification of White Dwarfs in the New Luyten Two-Tenths Survey
DOI: 10.1086/374772 Bibcode: 2003ApJ...586L..95V

Vennes, Stéphane; Kawka, Adela

We spectroscopically identify New Luyten Two-Tenths (NLTT) stars from the reduced proper-motion diagram of Salim & Gould. Five out of 16 objects investigated are identified as white dwarfs: four hydrogen-rich DA stars (NLTT 8581, NLTT 31748, NLTT 53177, and NLTT 56805) and one helium-rich (NLTT 8435). The properties of the stars are further co…

2003 The Astrophysical Journal
IUE 17
Detection of Far-Infrared Features in Star-Forming Regions
DOI: 10.1086/346178 Bibcode: 2003ApJ...585..872O

Onaka, Takashi; Okada, Yoko

We report the detection of a feature at 65 µm and a broad feature around 100 µm in the far-infrared spectra of the diffuse emission from two active star-forming regions, the Carina Nebula and Sharpless 171. The features are seen in the spectra over a wide area of the observed regions, indicating that the carriers are fairly ubiquitous …

2003 The Astrophysical Journal
ISO 17
An X-Ray Image of the Composite Supernova Remnant SNR G16.7+0.1
DOI: 10.1086/375838 Bibcode: 2003ApJ...592..941H

Gotthelf, E. V.; Agüeros, Marcel A.; Helfand, David J.

We have observed the Galactic supernova remnant G16.7+0.1 for 13 ks using the EPIC cameras on board the XMM-Newton X-Ray Observatory, producing the first X-ray image of the remnant. This composite radio remnant has a core radio flux density of only 100 mJy, making it one of the faintest radio synchrotron nebulae yet detected, although the core-to-…

2003 The Astrophysical Journal
XMM-Newton 17
Solving the Discrepancy between the Extreme-Ultraviolet and Microwave Observations of the Quiet Sun
DOI: 10.1086/374811 Bibcode: 2003ApJ...589.1054L

Landi, E.; Chiuderi Drago, F.

The aim of the present work is to understand the origin of the long-standing discrepancy between the EUV/UV-based predictions of the quiet-Sun microwave spectrum and the observed one. We compare accurate measurements of the quiet-Sun microwave brightness temperature (Tb) with theoretical calculations obtained by using the differential e…

2003 The Astrophysical Journal
SOHO 17
Hα, Extreme-Ultraviolet, and Microwave Observations of the 2000 March 22 Solar Flare and Spontaneous Magnetic Reconnection
DOI: 10.1086/346024 Bibcode: 2003ApJ...585..524L

Gallagher, Peter T.; Choe, G. S.; Nita, Gelu M. +4 more

The evolution of a GOES class X1.1 solar flare, which occurred in NOAA Active Region 8910 on 2000 March 22, is discussed using observations from the Owens Valley Solar Array (OVSA), Big Bear Solar observatory (BBSO), Transition Region and Coronal Explorer (TRACE), and the Michelson Doppler Imager (MDI) on board Solar and Heliospheric Observatory (…

2003 The Astrophysical Journal
SOHO 17