Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Bosch, G. L."'
We present the measurements of gas and stellar velocity dispersions in 17 circumnuclear star-forming regions (CNSFRs) and the nuclei of three barred spiral galaxies: NGC2903, NGC3310 and NGC3351 from high dispersion spectra. The stellar dispersions h
Externí odkaz:
http://arxiv.org/abs/1205.3704
We have studied the properties of an infrared cluster embedded in the gas and dust of the southern part of the Carina Nebula (NGC 3372), where the probable existence of current star formation has already been predicted. We used mid-infrared (A & C ba
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410185
Publikováno v:
Mon.Not.Roy.Astron.Soc.333:202,2002
We present a new optical spectroscopic study of the O-type binary HD 165052 based on high- and intermediate-resolution CCD observations. We re-investigated the spectral classification of the binary components, obtaining spectral types of O6.5 V and O
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205106
Publikováno v:
Mon.Not.Roy.Astron.Soc. 329 (2002) 481
We have obtained accurate CCD narrow band H_beta and H_alpha photometry of Giant HII Regions in M 33, NGC 6822 and M 101. Comparison with previous determinations of emission line fluxes show large discrepancies; their probable origins are discussed.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0109421
Akademický článek
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Autor:
Cellone, S. A., Barbá, R. H., Niemelä, V., Feinstein, C., Morrell, N., Cerruti, M. A., García, L. G., Moffat, A. F. J., Baume, G., Brandi, E. E., Orsatti, A. M., Vega, I., Martínez, R. E., Waldhausen, S., Bosch, G. L., Méndez, R. M., Ostrov, P., Eduardo Fernández Lajús
Publikováno v:
ResearcherID
Scopus-Elsevier
Scopus-Elsevier
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::06ae39edb77ff4520b22235631272c63
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=ORCID&SrcApp=OrcidOrg&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:A1996BH25G00025&KeyUID=WOS:A1996BH25G00025
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=ORCID&SrcApp=OrcidOrg&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:A1996BH25G00025&KeyUID=WOS:A1996BH25G00025
Autor:
Sean M. Dougherty, Roland Kothes
The goal of this study is to determine a distance to Westerlund 1 independent of the characteristics of the stellar population and to study its neutral environment, using observations of atomic hydrogen. The HI observations are taken from the Souther
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04019b64c71bc0f8c7b6c03104075331