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Identification of the Low-Mass X-Ray Binary and Faint X-Ray Sources in NGC 6652
Heinke, C. O.; Grindlay, J. E.; Edmonds, P. D.
We have detected three new X-ray point sources, in addition to the known low-mass X-ray binary (LMXB) X1832-330, in the globular cluster NGC 6652 with a Chandra 1.6 ks HRC-I exposure. Star 49 (MV~4.7), suggested by Deutsch and coworkers as the optical candidate for the LMXB, is identified (<0.3") not with the LMXB, but with another, …
Heating of Coronal Holes and Generation of the Solar Wind by Ion-Cyclotron Resonance
Isenberg, Philip A.
We discuss a new model to describe the heating of the magnetically open solar corona and the acceleration of the fast solar wind by the cyclotron resonant interaction of coronal ions with ion-cyclotron waves. This `kinetic shell' model includes important details of the wave-particle interaction which are not present in most other treatments. In th…
An Upper Mass Limit for the Progenitor of the Type II-P Supernova SN 1999gi
Smartt, Stephen J.; Gilmore, Gerard F.; Trentham, Neil +2 more
Masses and progenitor evolutionary states of Type II supernovae remain almost unconstrained by direct observations. Only one robust observation of a progenitor (SN 1987A) and one plausible observation (SN 1993J) are available. Neither matched theoretical predictions, and in this Letter we report limits on a third progenitor (SN 1999gi). The Hubble…
Observational Constraints on the Abundance and Evolution of ``XCN'' in Interstellar Grain Mantles
Whittet, D. C. B.; Boogert, A. C. A.; Pendleton, Y. J. +3 more
The 4.62 µm ``XCN'' absorption feature, attributed to CN-bearing molecules in solids, is potentially an important diagnostic of the evolution of organic matter in the interstellar medium and the envelopes of newly formed stars. We report quantitative limits on the strength of this feature in the diffuse interstellar medium toward the reddene…
The Star Formation History of LGS 3
Dolphin, Andrew E.; Miller, Bryan W.; Lee, Myung Gyoon +2 more
We have determined the distance and star formation history of the Local Group dwarf galaxy LGS 3 from deep Hubble Space Telescope WFPC2 observations. LGS 3 is intriguing because ground-based observations showed that, while its stellar population is dominated by old, metal-poor stars, there is a handful of young, blue stars. Also, the presence of H…
Far-Infrared Detection of H3O+ in Sagittarius B2
Cernicharo, José; Goicoechea, Javier R.
We report the first far-infrared detection of the hydronium ion (H3O+) toward the Sagittarius B2 molecular cloud, near the Galactic center. Using the Infrared Space Observatory Long-Wavelength Spectrometer, we have detected three lines arising from the ν2 ground-state inversion mode (0+-->0-
Hα Proxies for EIT Crinkles: Further Evidence for Preflare ``Breakout''-Type Activity in an Ejective Solar Eruption
Qiu, Jiong; Wang, Haimin; Moore, Ronald L. +1 more
We present Hα observations from Big Bear Solar Observatory of an eruptive flare in NOAA Active Region 8210, occurring near 22:30 UT on 1998 May 1. Previously, using the EUV Imaging Telescope (EIT) on the SOHO spacecraft, we found that a pattern of transient, localized brightenings, which we call ``EIT crinkles,'' appears in the neighborhood of the…
STIS Echelle Observations of the Intrinsic UV Absorption in the Seyfert 1 Galaxy NGC 3783
Kraemer, S. B.; Crenshaw, D. M.; Gabel, J. R.
We present observations of the UV absorption lines in the Seyfert 1 galaxy NGC 3783, obtained with the medium resolution (λ/Δλ~40,000) echelle gratings of the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST). The spectra reveal the presence of three kinematic components of absorption in Lyα, C IV, and N V, at radial …
Cassiopeia A dust composition and heating
Pantin, E.; Lagage, P. O.; Douvion, T.
Material ejected by a supernova is directly observed in the form of Fast Moving Knots (FMK's) in the Cassiopeia A supernova remnant. Part of this material has condensed into dust. In this paper, by fitting the ISO mid-infrared emission of the dust, we derive the dust composition and discuss the dust heating. The dust is found to be made mainly of …
Wind circulation in selected rotating magnetic early-B stars
Smith, M. A.; Groote, D.
The rotating magnetic B stars are a class of variables consisting of He-strong and some beta Cep stars which have oblique dipolar magnetic fields. Such stars develop co-rotating, torus-shaped clouds by channeling wind particles from their magnetic poles to circumstellar regions centered around the plane of their magnetic equators. The rotation of …