Search Publications

Evidence for Expanding Superbubbles in a Galaxy at z=0.7443
DOI: 10.1086/321689 Bibcode: 2001ApJ...557..761B

Vogt, Steven S.; Charlton, Jane C.; Churchill, Christopher W. +1 more

The intervening z=0.7443 Mg II absorption system in the spectrum of MC 1331+170 shows an unusual series of line pairs, each with Δv~30 km s-1. These lines could be explained as the shells of expanding superbubbles residing in the outer regions of an edge-on spiral galaxy visible in the optical image of the MC 1331+170 field. The color a…

2001 The Astrophysical Journal
eHST 29
Multicolor Observations of the Hubble Deep Field South
DOI: 10.1086/323544 Bibcode: 2001AJ....122.2190V

Fontana, Adriano; Grazian, Andrea; Bianchi, Simone +6 more

We present a deep multicolor (U, B, V, I, Js, H, Ks) catalog of galaxies in the Hubble Deep Field South, based on observations obtained with the HST WFPC2 in 1998 and VLT-ISAAC in 1999. The photometric procedures were tuned to derive a catalog optimized for the estimation of photometric redshifts. In particular we adopted a ``conservative'' detect…

2001 The Astronomical Journal
eHST 29
Multicolor photometry of the Vela pulsar
DOI: 10.1051/0004-6361:20010951 Bibcode: 2001A&A...376..213M

Caraveo, P. A.; Mignani, R. P.

Multicolor photometry of the Vela pulsar (PSR B0833-45), updated by recent HST/WFPC2 observations obtained in the 555W, 675W and 814W filters, is presented. The available data provide the best characterization so far of the pulsar spectral shape, which is dominated by a flat power law continuum with spectral index alpha = -0.2 +/- 0.2, consistent …

2001 Astronomy and Astrophysics
eHST 29
Evolution of the dust mass loss with luminosity along the giant branch of the globular cluster 47 Tucanae
DOI: 10.1051/0004-6361:20010361 Bibcode: 2001A&A...372...85R

Jorissen, A.; Ramdani, A.

The present paper investigates the properties of the dust mass loss in stars populating the giant branch of the globular cluster 47 Tuc, by combining ISOCAM and DENIS data. Raster maps of 5 fields covering areas ranging from 4x4 to 15x15 arcmin2 at different distances from the center of the cluster have been obtained with ISOCAM at 11.5…

2001 Astronomy and Astrophysics
ISO 29
Compact Star Clusters in M81. I. Data from Hubble Space Telescope Wide Field Planetary Camera 2 Imaging
DOI: 10.1086/322127 Bibcode: 2001AJ....122.1330C

Chandar, Rupali; Ford, Holland C.; Tsvetanov, Zlatan

In this paper, we present the discovery of 114 compact star clusters in the nearby spiral galaxy M81 from B-, V-, and I-band Hubble Space Telescope Wide Field Planetary Camera 2 imaging in eight fields, covering a total area of ~40 arcmin2. The fields sample a variety of environments (both spiral and interarm regions), as well as a rang…

2001 The Astronomical Journal
eHST 29
The galactic mass injection from cool stellar winds of the 1 to 2.5 Msun stars in the solar neighbourhood
DOI: 10.1051/0004-6361:20000282 Bibcode: 2001A&A...366..913S

Schröder, K. -P.; Sedlmayr, E.

We have computed synthetic stellar samples and HR diagrams on the basis of a fine-meshed, consistent grid of evolution tracks for given IMF and SFR(t). In order to model the galactic disk stellar component (single stars only) and to derive its IMF and apparent SFR(t), we selected the synthetic sample which is the best fit to the observed distribut…

2001 Astronomy and Astrophysics
Hipparcos 29
A far infrared view of low mass star formation in the Cederblad 110 nebula of Chamaeleon I
DOI: 10.1051/0004-6361:20000401 Bibcode: 2001A&A...367..311L

Lemke, D.; Lehtinen, K.; Mattila, K. +1 more

The Cederblad 110 reflection nebula contains several young stellar objects previously discovered by IRAS and sub-mm observations. This cluster was revisited with ISO's FIR cameras and mapped with higher spatial resolution. All sources were also mapped for the first time near the maximum of their spectral energy distribution at 200 mu m. In additio…

2001 Astronomy and Astrophysics
ISO 29
The structure of the Akn 120 emitting region: The line shapes and long-term Hβ line profile variation
DOI: 10.1051/0004-6361:20000500 Bibcode: 2001A&A...367..780P

Bon, E.; Stanić, N.; Kubičela, A. +1 more

To investigate the structure of the Akn 120 emitting region we have analysed the spectral line profiles of Halpha, Hbeta, Lyalpha, C III[1909], C IV[1549] and Mg II[2798] lines using a Gaussian-decomposition approach. The decomposed shape of the Akn 120 lines indicates three separated broad line-emitting regions, i…

2001 Astronomy and Astrophysics
eHST 29
Measuring Sizes of Marginally Resolved Young Globular Clusters with the Hubble Space Telescope
DOI: 10.1086/324417 Bibcode: 2001PASP..113.1522C

Holtzman, Jon A.; Carlson, Matthew N.

We present a method for deriving sizes of marginally resolved star clusters from Hubble Space Telescope/WFPC2 observations by fitting King models to observations. We describe results both on simulated images and on observations of young compact clusters in NGC 3597 and NGC 1275. From the simulations, we find that we can measure King model concentr…

2001 Publications of the Astronomical Society of the Pacific
eHST 28
EUV Sprays: Jet-like eruptive activity on the solar limb
DOI: 10.1051/0004-6361:20011171 Bibcode: 2001A&A...379..324H

Harrison, R. A.; Bryans, P.; Bingham, R.

Jet-like eruptive events have been detected in the extreme ultraviolet (EUV) observations from the Solar and Heliospheric Observatory (SOHO) spacecraft. Some jet-like events are shown and for one event, that of January 22 2000, we provide a detailed analysis of the EUV observations. The January 22 observation was part of an on-going campaign to ob…

2001 Astronomy and Astrophysics
SOHO 28