Search Publications

Spatial Separation of the 3.29 Micron Emission Feature and Associated 2 Micron Continuum in NGC 7023
DOI: 10.1086/378630 Bibcode: 2003ApJ...599..312A

Sellgren, K.; An, Jin H.

We present a new 0.9" resolution 3.29 µm narrowband image of the reflection nebula NGC 7023. We find that the 3.29 µm infrared emission feature (IEF) in NGC 7023 is brightest in narrow filaments northwest of the illuminating star HD 200775. These filaments have been previously seen in images of extended red emission, K', near-infrared …

2003 The Astrophysical Journal
eHST 25
Interaction and Dynamics of the Photospheric Network Magnetic Elements
DOI: 10.1023/A:1023928212747 Bibcode: 2003SoPh..213..231R

Tarbell, T. D.; Shine, R.; Ryutova, M.

Small-scale magnetic elements in the quiet photospheric network are believed to play a key role in the energy flow from the solar surface to upper layers of atmosphere. Their intense hydro-magnetic activity includes merging and fragmentation of same polarity fluxes, `total' or partial cancellation of neighboring flux elements of opposite polarity,…

2003 Solar Physics
SOHO 24
Determination of the solar wind slowdown near solar maximum
DOI: 10.1029/2002JA009322 Bibcode: 2003JGRA..108.1058W

Wang, C.; Richardson, J. D.

The magnitude of the solar wind speed decrease from the inner to the outer heliosphere provides important information about the interaction of the heliosphere with the local interstellar medium (LISM), leading to better estimates of the size and shape of the heliosphere and of the LISM density. In this study we combine observations from multiple s…

2003 Journal of Geophysical Research (Space Physics)
Ulysses 24
X-ray emission line gas in the LINER galaxy M 81
DOI: 10.1051/0004-6361:20021896 Bibcode: 2003A&A...400..145P

Page, M. J.; Branduardi-Raymont, G.; Zane, S. +5 more

We present the soft X-ray spectrum of the LINER galaxy M 81 derived from a long observation with the XMM-Newton RGS. The spectrum is dominated by continuum emission from the active nucleus, but also contains emission lines from Fe L, and H-like and He-like N, O, and Ne. The emission lines are significantly broader than the RGS point-source spectra…

2003 Astronomy and Astrophysics
XMM-Newton 24
A multi-wavelength test of the FR I-BL Lac unifying model
DOI: 10.1051/0004-6361:20030417 Bibcode: 2003A&A...403..889T

Capetti, A.; Chiaberge, M.; Celotti, A. +2 more

We collect multi-wavelength measurements of the nuclear emission of 20 low luminosity FR I radio-galaxies to test the viability of the FR I-BL Lac unifying model. Although poorly sampled, the Spectral Energy Distributions (SED) of FR Is are consistent with the double peaked shape characteristic of BL Lacs. Furthermore while the distribution of the…

2003 Astronomy and Astrophysics
eHST 24
Solar magnetic field reversal as seen at Ulysses
DOI: 10.1029/2003GL017204 Bibcode: 2003GeoRL..30.8028J

Balogh, André; Smith, Edward J.; Jones, Geraint H.

The rapid motion of the Ulysses spacecraft from high southern to high northern latitudes in 2000-2001 provided an excellent opportunity to make inferences regarding the solar magnetic dipole's behaviour around solar maximum. A simple dipole model is fitted to Ulysses measurements of the polarity of the heliospheric magnetic field mapped back to th…

2003 Geophysical Research Letters
Ulysses 24
XMM-Newton observations of the polars EV UMa, RX J1002-19 and RX J1007-20
DOI: 10.1046/j.1365-8711.2003.06045.x Bibcode: 2003MNRAS.338..219R

Cropper, Mark; Ramsay, Gavin

We present XMM-Newton data of three strongly magnetic cataclysmic variables (polars) EV UMa, RX J1002-19 and RX J1007-20. These include the polar with the shortest orbital period (EV UMa) and the polar with one of the highest magnetic field strengths (RX J1007-20). They exhibit a range of X-ray spectral characteristics which are consistent with th…

2003 Monthly Notices of the Royal Astronomical Society
XMM-Newton 24
Far UV spectroscopy of the circumstellar environment of the Herbig Be stars HD 259431 and HD 250550
DOI: 10.1051/0004-6361:20031151 Bibcode: 2003A&A...410..175B

Deleuil, M.; Bouret, J. -C.; Catala, C. +2 more

We present an analysis of FUSE spectra of HD 259431 and HD 250550, two young Herbig Be stars. Numerous absorption lines of H_2 are seen in the spectrum of each star, revealing large amounts of this gas on the lines of sight. In addition, absorption lines from atomic species in different ionization and excitation states are also identified. We demo…

2003 Astronomy and Astrophysics
IUE 24
UV(IUE) spectra of hot post-AGB candidates
DOI: 10.1051/0004-6361:20030996 Bibcode: 2003A&A...407.1007G

Parthasarathy, M.; Gauba, G.

Analysis of the low resolution UV(IUE) spectra (1150 to 3200 Å) of 15 hot post-AGB candidates is presented. The UV(IUE) spectra of 10 stars suggest partial obscuration of the hot stars due to circumstellar dust. The reddened continua of these 10 stars were used to model and estimate the circumstellar extinction. The circumstellar extinction law wa…

2003 Astronomy and Astrophysics
IUE 24
Hubble Space Telescope STIS Observations of Comet 19P/Borrelly during the Deep Space 1 Encounter
DOI: 10.1086/375752 Bibcode: 2003AJ....126..444W

Stern, S. A.; Weaver, H. A.; Parker, J. Wm.

In support of the NASA Deep Space 1 (DS1) mission to comet 19P/Borrelly, we obtained Hubble Space Telescope (HST) images and ultraviolet (UV) spectra of the comet near the time of the DS1 flyby in 2001 September. The HST data provide context information on 19P/Borrelly's circumnuclear dust environment, the rotational period and rotational phase of…

2003 The Astronomical Journal
eHST 24