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The Internal Structure and Formation of Early-Type Galaxies: The Gravitational Lens System MG 2016+112 at z = 1.004
DOI: 10.1086/341216 Bibcode: 2002ApJ...575...87T

Treu, Tommaso; Koopmans, Léon V. E.

We combine our recent measurements of the velocity dispersion and the surface brightness profile of the lens galaxy D in the system MG 2016+112 (z=1.004) with constraints from gravitational lensing to study its internal mass distribution. We find the following: (1) dark matter accounts for more than 50% of the total mass within the Einstein radius…

2002 The Astrophysical Journal
eHST 244
A New Spectral Classification System for the Earliest O Stars: Definition of Type O2
DOI: 10.1086/339831 Bibcode: 2002AJ....123.2754W

Walborn, Nolan R.; Parker, Joel Wm.; Drissen, Laurent +7 more

High-quality, blue-violet spectroscopic data are collected for 24 stars that have been classified as type O3 and that display the hallmark N IV and N V lines. A new member of the class is presented; it is the second known in the Cyg OB2 association, and only the second in the northern hemisphere. New digital data are also presented for several of …

2002 The Astronomical Journal
eHST 241
Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. II. Kinematic Analysis and Dynamical Modeling
DOI: 10.1086/344584 Bibcode: 2002AJ....124.3270G

Gerssen, Joris; van der Marel, Roeland P.; Gebhardt, Karl +3 more

We have used the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST) to obtain high spatial resolution spectroscopy of the central region of the dense globular cluster M15. The observational strategy and data reduction were described in Paper I of this series. Here we analyze the extracted spectra with a cross-correlati…

2002 The Astronomical Journal
eHST 240
The M 81 group of galaxies: New distances, kinematics and structure
DOI: 10.1051/0004-6361:20011741 Bibcode: 2002A&A...383..125K

Sarajedini, A.; Dolphin, A. E.; Grebel, E. K. +7 more

We present Hubble Space Telescope/WFPC2 images of the galaxies NGC 2366, NGC 2976, NGC 4236, IC 2574, DDO 53, DDO 82, DDO 165, Holmberg I, Holmberg II, Holmberg IX, K52, K73, BK3N, Garland, and A0952+69 in the M 81 complex. Their true distance moduli, derived from the brightness of the tip of the red giant branch, lie in the range of 27fm 52 (NGC …

2002 Astronomy and Astrophysics
eHST 239
Interacting Coronal Mass Ejections and Solar Energetic Particles
DOI: 10.1086/341601 Bibcode: 2002ApJ...572L.103G

Kaiser, M. L.; Howard, R. A.; Gopalswamy, N. +5 more

We studied the association between solar energetic particle (SEP) events and coronal mass ejections (CMEs) and found that CME interaction is an important aspect of SEP production. Each SEP event was associated with a primary CME that is faster and wider than average CMEs and originated from west of E45°. For most of the SEP events, the primary CME…

2002 The Astrophysical Journal
SOHO 237
The Palomar/MSU Nearby Star Spectroscopic Survey. IV. The Luminosity Function in the Solar Neighborhood and M Dwarf Kinematics
DOI: 10.1086/343777 Bibcode: 2002AJ....124.2721R

Hawley, Suzanne L.; Gizis, John E.; Reid, I. Neill

We have used new astrometric and spectroscopic observations to refine the volume-complete sample of M dwarfs defined in previous papers in this series. With the addition of Hipparcos astrometry, our revised VC2 sample includes 558 main-sequence stars in 448 systems. Analysis of that data set shows no evidence of any systematic kinematic…

2002 The Astronomical Journal
Hipparcos 236
Measuring the redshift evolution of clustering: the Hubble Deep Field South
DOI: 10.1046/j.1365-8711.2002.04988.x Bibcode: 2002MNRAS.329..355A

Colombi, S.; Matarrese, S.; Fontana, A. +6 more

We present an analysis of the evolution of galaxy clustering in the redshift interval 0<=z<=4.5 in the Hubble Deep Field South (HDF-South). The HST optical data are combined with infrared ISAAC/VLT observations, and photometric redshifts are used for all the galaxies brighter than IAB<=27.5. The clustering signal is obtained in…

2002 Monthly Notices of the Royal Astronomical Society
eHST 231
Planetary Nebulae as Standard Candles. XII. Connecting the Population I and Population II Distance Scales
DOI: 10.1086/342180 Bibcode: 2002ApJ...577...31C

Ciardullo, Robin; Durrell, Patrick R.; Feldmeier, John J. +3 more

We report the results of [O III] λ5007 surveys for planetary nebulae (PNe) in six galaxies: NGC 2403, NGC 3115, NGC 3351, NGC 3627, NGC 4258, and NGC 5866. Using on-band/off-band [O III] λ5007 images, as well as images taken in Hα, we identify samples of PNe in these galaxies and derive their distances using the planetary nebula luminosity functio…

2002 The Astrophysical Journal
eHST 231
Hot Coronal Loop Oscillations Observed by SUMER: Slow Magnetosonic Wave Damping by Thermal Conduction
DOI: 10.1086/345548 Bibcode: 2002ApJ...580L..85O

Ofman, L.; Wang, Tongjiang

Recently, strongly damped Doppler shift oscillations of hot (T>6 MK) coronal loops were observed with the Solar Ultraviolet Measurement of Emitted Radiation (SUMER) spectrometer on board the Solar and Heliospheric Observatory. The oscillations are interpreted as signatures of slow-mode magnetosonic waves excited impulsively in the loops. Using …

2002 The Astrophysical Journal
SOHO 229
Solar Phenomena Associated with ``EIT Waves''
DOI: 10.1086/339402 Bibcode: 2002ApJ...569.1009B

Thompson, B. J.; Biesecker, D. A.; Vourlidas, A. +2 more

In an effort to understand what an ``EIT wave'' is and what its causes are, we have looked for correlations between the initiation of EIT waves and the occurrence of other solar phenomena. An EIT wave is a coronal disturbance, typically appearing as a diffuse brightening propagating across the Sun. A catalog of EIT waves, covering the period from …

2002 The Astrophysical Journal
SOHO 228