Search Publications

The Spectral Components of SS 433
DOI: 10.1086/338335 Bibcode: 2002ApJ...566.1069G

Wang, Z.; Gies, D. R.; McSwain, M. V. +3 more

We present results from new optical and UV spectroscopy of the unusual binary system SS 433, and we discuss the relationship of the particular spectral components that we observe to the properties of the binary. These spectral components include1. The continuum spectrum, which we associate with flux from the super-Eddington accretion disk and the …

2002 The Astrophysical Journal
IUE eHST 73
Hubble Space Telescope Spectra of GW Librae: A Hot Pulsating White Dwarf in a Cataclysmic Variable
DOI: 10.1086/342916 Bibcode: 2002ApJ...575L..79S

Szkody, Paula; Howell, Steve B.; Sion, Edward M. +1 more

We have obtained Hubble Space Telescope UV spectra of the white dwarf in GW Lib, the only known nonradially pulsating white dwarf in a cataclysmic variable and the first known DAZQ variable. The UV light curve reveals large-amplitude (10%) pulsations in the UV with the same periods (646, 376, and 237 s) as those seen at optical wavelengths, but th…

2002 The Astrophysical Journal
eHST 73
X-ray evidence for spectroscopic diversity of type Ia supernovae:. XMM observation of the elemental abundance pattern in M 87
DOI: 10.1051/0004-6361:20011477 Bibcode: 2002A&A...381...21F

Finoguenov, A.; Böhringer, H.; Arnaud, M. +2 more

We present the results of a detailed element abundance study of hot gas in M 87, observed by XMM-Newton. We choose two radial bins, 1'-3' and 8'-16' (8'-14' for EMOS; hereafter the central and the outer zones), where the temperature is almost constant, to carry out the detailed abundance measurements of O, Ne, Mg, Si, S, Ar, Ca, Fe and Ni using EP…

2002 Astronomy and Astrophysics
XMM-Newton 72
The Heavy-Element Enrichment of Lyα Clouds in the Virgo Supercluster
DOI: 10.1086/341338 Bibcode: 2002ApJ...575..697T

Gull, T. R.; Davé, R.; Heap, S. R. +11 more

Using high signal-to-noise ratio echelle spectra of 3C 273 obtained with the Space Telescope Imaging Spectrograph (resolution of 7 km s-1 FWHM), we constrain the metallicities of two Lyα clouds in the vicinity of the Virgo Cluster. We detect C II, Si II, and Si III absorption lines in the Lyα absorber at zabs=0.00530. Previou…

2002 The Astrophysical Journal
eHST 72
Revised Coordinates and Proper Motions of the Stars in the Luyten Half-Second Catalog
DOI: 10.1086/340115 Bibcode: 2002ApJS..141..187B

Bakos, Gáspár Á.; Sahu, Kailash C.; Németh, Péter

We present refined coordinates and proper-motion data for the high proper-motion (HPM) stars in the Luyten Half-Second (LHS) catalog. The positional uncertainty in the original Luyten catalog is typically greater than 10" and is often greater than 30". We have used the digital scans of the POSS I and POSS II plates to derive more accurate position…

2002 The Astrophysical Journal Supplement Series
Hipparcos 72
A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters - II. A search for gravitationally lensed EROs *
DOI: 10.1046/j.1365-8711.2002.04984.x Bibcode: 2002MNRAS.330....1S

Kneib, J. -P.; Ivison, R. J.; Smith, Graham P. +7 more

We present the results of a survey for extremely red objects (EROs) undertaken in the fields of 10 massive galaxy cluster lenses at , combining sensitive, high-resolution Hubble Space Telescope imaging with deep, half-arcsecond K -band imaging from UKIRT. We detect 60 EROs with , of which 26 have in a total image-plane survey area of 49arcmin

2002 Monthly Notices of the Royal Astronomical Society
eHST 72
Interplanetary phenomena associated with very intense geomagnetic storms
DOI: 10.1016/S1364-6826(01)00082-7 Bibcode: 2002JASTP..64..173G

Schwenn, R.; Tsurutani, B. T.; Lepping, R. P. +1 more

The dominant interplanetary phenomena that are frequently associated with intense magnetic storms are the interplanetary manifestations of fast coronal mass ejections (CMEs). Two such interplanetary structures, involving an intense and long duration Bs component of the IMF are: the sheath region behind a fast forward interplanetary shoc…

2002 Journal of Atmospheric and Solar-Terrestrial Physics
SOHO 72
What Fraction of the Young Clusters in the Antennae Galaxies Are ``Missing''?
DOI: 10.1086/341822 Bibcode: 2002AJ....124.1418W

Whitmore, Bradley C.; Zhang, Qing

A reexamination of the correspondence between 6 cm radio continuum sources and young star clusters in the Antennae galaxies indicates that ~85% of the strong thermal sources have optical counterparts, once the optical image is shifted 1.2" to the southwest. A sample of 37 radio-optical matches are studied in detail, showing correlations between ra…

2002 The Astronomical Journal
eHST 72
A Study of π Aquarii during a Quasi-normal Star Phase: Refined Fundamental Parameters and Evidence for Binarity
DOI: 10.1086/340751 Bibcode: 2002ApJ...573..812B

Bjorkman, Karen S.; Miroshnichenko, Anatoly S.; McDavid, David +1 more

We present the results of recent multicolor photometric and high-resolution spectroscopic observations of the bright Be star π Aqr. Observational data collected from the literature were used to study the star's variations over the last four decades. The star is identified with the IR sources F22227+0107 in the IRAS Faint Point Source Catalog and M…

2002 The Astrophysical Journal
IUE 72
PKS 1830-211: A Face-on Spiral Galaxy Lens
DOI: 10.1086/341265 Bibcode: 2002ApJ...575..103W

Rix, Hans-Walter; Winn, Joshua N.; Kochanek, Christopher S. +3 more

We present new Hubble Space Telescope images of the gravitational lens PKS 1830-211, which allow us to characterize the lens galaxy and update the determination of the Hubble constant (H0) from this system. The I-band image shows that the lens galaxy is a face-on spiral galaxy with clearly delineated spiral arms. The southwestern image …

2002 The Astrophysical Journal
eHST 71