Search Publications

An XMM-Newton Observation of the Luminous Seyfert 1 Galaxy Markarian 509
DOI: 10.1086/322315 Bibcode: 2001ApJ...559..181P

Reeves, James; Nayakshin, Sergei; O'Brien, Paul +3 more

We present the spectral analysis of an early XMM-Newton observation of the luminous Seyfert 1 galaxy Mrk 509. We find the hard (2-10 keV) continuum slope, including reflection, to be somewhat flatter (Γ=1.75) than that of a typical broad-line Seyfert 1 galaxy. The most obvious feature in the hard X-ray spectrum is a narrow emission line near 6.4 k…

2001 The Astrophysical Journal
XMM-Newton 89
XMM-Newton observation of an unusual iron line in the quasar Markarian 205
DOI: 10.1051/0004-6361:20000424 Bibcode: 2001A&A...365L.134R

Boller, Th.; O'Brien, P. T.; Reeves, J. N. +5 more

XMM-Newton observations of the low luminosity, radio-quiet quasar Markarian 205 have revealed a unique iron K emission line profile. In marked contrast to the broad and redshifted iron K line commonly seen in ASCA observations of Seyfert 1 galaxies, we find that a substantial amount of the line flux in Mrk 205 occurs above the neutral line energy …

2001 Astronomy and Astrophysics
XMM-Newton 89
A K-band-Selected Photometric Redshift Catalog in the Hubble Deep Field South: Sampling the Rest-Frame V Band to z =3
DOI: 10.1086/323542 Bibcode: 2001AJ....122.2205R

Franx, Marijn; Labbé, Ivo; van Dokkum, Pieter +7 more

We present the first results from the Faint Infra-Red Extragalactic Survey of the Hubble Deep Field South (HDF-S). Using a combination of deep near-infrared (NIR) data obtained with the Infrared Spectrograph and Array Camera at the VLT and the WFPC2 Hubble Space Telescope data, we construct a K-band-selected sample which is 50% and 90% complete fo…

2001 The Astronomical Journal
eHST 89
Multiwavelength analyses of the extraordinary nova LMC 1991*
DOI: 10.1046/j.1365-8711.2001.03960.x Bibcode: 2001MNRAS.320..103S

Della Valle, M.; Baron, E.; Shore, S. N. +3 more

LMC 91 was a very fast, classical nova and the brightest nova ever observed in the Large Magellanic Cloud. It was extensively observed during both its early optically thick and its nebular evolution in the optical and UV wavelength regions. We successfully fit all the optically thick spectra using a grid of spherically symmetric, non-LTE, line-bla…

2001 Monthly Notices of the Royal Astronomical Society
IUE 88
Spectroscopic Diagnostics of Nanoflare-heated Loops
DOI: 10.1086/320666 Bibcode: 2001ApJ...553..440K

Klimchuk, J. A.; Cargill, P. J.

To evaluate the usefulness of spectroscopic techniques for diagnosing realistic solar plasmas and to better understand the physical origin of coronal heating, we have simulated observations of model coronal loops that are heated randomly and impulsively by nanoflares. We find that the emission measures, densities, and filling factors that are infe…

2001 The Astrophysical Journal
SOHO 88
Far-Ultraviolet and Hα Imaging of Nearby Spiral Galaxies: The OB Stellar Population in the Diffuse Ionized Gas
DOI: 10.1086/322422 Bibcode: 2001ApJ...559..878H

Hoopes, Charles G.; Bothun, Gregory D.; Walterbos, René A. M.

We have compared Hα and far-ultraviolet (FUV) images of 10 nearby spirals, with the goal of understanding the contribution of field OB stars to the ionization of the diffuse ionized gas (DIG) in spiral galaxies. The FUV images were obtained by the Ultraviolet Imaging Telescope (UIT), and the Hα images were obtained using various ground-based teles…

2001 The Astrophysical Journal
eHST 88
XMM-Newton observations of NGC 253: Resolving the emission components in the disk and nuclear area
DOI: 10.1051/0004-6361:20000068 Bibcode: 2001A&A...365L.174P

Pietsch, W.; Read, A. M.; Ptak, A. +12 more

We describe the first XMM-Newton observations of the starburst galaxy NGC 253. As known from previous X-ray observations, NGC 253 shows a mixture of extended (disk and halo) and point-source emission. The high XMM-Newton throughput allows a detailed investigation of the spatial, spectral and variability proper…

2001 Astronomy and Astrophysics
XMM-Newton 87
NGC 1614: A Laboratory for Starburst Evolution
DOI: 10.1086/318282 Bibcode: 2001ApJ...546..952A

Rieke, G. H.; Alonso-Herrero, A.; Quillen, A. C. +2 more

The modest extinction and reasonably face-on viewing geometry make the luminous infrared galaxy NGC 1614 an ideal laboratory for the study of a powerful starburst. Hubble Space Telescope/near-infrared camera and multiobject spectrometer (NICMOS) observations show (1) deep CO stellar absorption, tracing a starburst nucleus about 45 pc in diameter (…

2001 The Astrophysical Journal
eHST 87
A two-Type Classification of Lasco Coronal Mass Ejection
DOI: 10.1023/A:1005284316619 Bibcode: 2001SSRv...95..147A

Andrews, M. D.; Howard, R. A.

The causes and origins of Coronal Mass Ejections (CMEs) remain among the outstanding questions in Space Physics. The observations of CMEs by the LASCO coronagraphs on SOHO suggest that there are two distinct types of CMEs. The two types of events can be most easily distinguished by examining height-time plots. The Type A (Acceleration) events prod…

2001 Space Science Reviews
SOHO 87
Hubble Space Telescope Proper-Motion Measurements of the η Carinae Nebula
DOI: 10.1086/319092 Bibcode: 2001ApJ...548L.207M

Davidson, Kris; Bally, John; Balick, Bruce +3 more

We present proper-motion measurements of the bipolar lobes and equatorial disk features ejected from η Carinae during the last century and deduce their relative ages in order to determine the likelihood of multiple ejection events. Hubble Space Telescope Wide Field Planetary Camera 2 images taken in 1994, 1995, and 1999 were compared, and the moti…

2001 The Astrophysical Journal
eHST 86