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UV through far-IR analysis of M81
The recent star formation (SF) in the early-type spiral galaxy M81 is characterized using imaging observations from the far-ultraviolet to the far-infrared. We compare these... -
NGC4395 light curves
A reverberation-mapping program on NGC 4395, the least luminous known Seyfert 1 galaxy, undertaken with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope... -
Star formation in Stephan's Quintet
We present the first Galaxy Evolution Explorer (GALEX) UV images of the well-known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission... -
Optical and IUE spectra of NGC 7026
We investigated spectroscopic data of the extended planetary nebula NGC 7026 in the wavelengths 3700-10050{AA}, secured with the Hamilton Echelle Spectrograph at Lick... -
EUV spectrum of solar active region from SERTS-97
Goddard Space Flight Center's Solar EUV Research Telescope and Spectrograph was flown on 1997 November 18, carrying an intensified CCD detector and a multilayer-coated toroidal... -
UV and optical line variations in {epsilon} Persei
The rapid variable star, {epsilon} Per (B0.5 IV-III), displays the largest amplitude profile fluctuations known among the growing number of massive, spectrum-variable stars.... -
AX Mon photometry and UV spectra
AX Monocerotis is a 232d, noneclipsing, interacting binary star that consists of a K giant, a Be-like giant, and a large amounts of circumstellar material. The K star is almost... -
Observations of H II Regions in M81
Images of the type Sab spiral galaxy M81 were obtained in far-UV and near-UV bands by the Ultraviolet Imaging Telescope (UIT) during the Astro-1 Spacelab mission of 1990... -
IMF from UV stellar photometry
UV stellar photometry is presented for 1563 stars within a 40' circular field in the LMC, excluding the 10'x10' field centered on R136 investigated earlier by Hill et al.... -
Pop I UV radiation models
This series of papers comprises a systematic exploration of the hypothesis that the far-ultraviolet radiation from star clusters and elliptical galaxies originates from... -
Positions, plx, & phot. from Gaia for Berkeley 39
We characterize blue straggler stars (BSSs) and yellow straggler stars (YSSs) of the open cluster (OC) Berkeley 39 using multiwavelength observations including the... -
U-SMAC II. FUV catalog of sources detected in SMC
The Small Magellanic Cloud (SMC) is an irregular dwarf galaxy that has recently undergone an interaction with the Large Magellanic Cloud. The young massive stars in the SMC... -
Dust clouds masses, color excesses and distances
We present a catalog of dust clouds at high Galactic latitude based on the Planck 857GHz dust emission data. Using a clustering hierarchical algorithm, 315 dust clouds at high... -
FUMES. III. HST/STIS measurements of 9 M-dwarfs
We obtained ultraviolet and optical spectra for nine M-dwarfs across a range of rotation periods to determine whether they showed stochastic intrinsic variability... -
3000-10700{AA} spectral cover of NGC 6153 with VLT
We study the kinematics of emission lines that arise from many physical processes in NGC6153 based upon deep, spatially resolved, high-resolution spectra acquired with the UVES... -
Accretion in 9 Orion OB1b T-Tauri stars
The coevolution of T-Tauri stars and their surrounding protoplanetary disks dictates the timescales of planet formation. In this paper, we present magnetospheric accretion and... -
HST photometry in 6 dwarf galaxies
We present a comprehensive study of young stellar populations in six dwarf galaxies in or near the Local Group: Phoenix, Pegasus, Sextans A, Sextans B, WLM, and NGC 6822. Their... -
Analysis of B6-A9 stars from INES UV spectra
Main-sequence (MS) and giant late-B and early-A type stars are the best targets for searching for nearby interstellar (IS) SiIV and CIV resonance lines because they are not able... -
UVOT imaging of M81 and Holmberg IX
We present Swift UV/Optical Telescope (UVOT) imaging of the galaxies M81 and Holmberg IX. We combine UVOT imaging in three near-ultraviolet (NUV) filters (uvw2: 1928{AA}; uvm2:... -
SDSS-ROSAT AGN data
Using a sample of 228 optically selected active galactic nuclei (AGNs) in the 0.01-6.3 redshift range with a high fraction of X-ray detections (81%-86%), we study the relation...
