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VBLUW-photometry of stars in small fields around 13 planetary nebulae
Observations of stars in small fields around 13 planetary nebulae, madeusing the Walraven five-channel VBLUW photometer, are presented anddescribed. The fields are found to have a radius of about 0.3 deg. Thefinding charts for the measured stars are given. It is shown that moststars are brighter than mV of about 14 mag and that the photometry hasan accuracy of better than 1 percent, except for stars that are observedwith short test-integrations and for stars fainter than mV of about 14mag. The photometric data for all stars are presented, together with alist of identifications and spectral types.
| Spectral classification from the ultraviolet line features of S2/68 spectra. II - Late B-type stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1977A&AS...30...71C&db_key=AST
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Cennet Kusu |
| Sað Açýklýk: | 15h30m49.18s |
| Yükselim: | -71°39'14.9" |
| Görünürdeki Parlaklýk: | 6.377 |
| Uzaklýk: | 322.581 parsek |
| özdevim Sað Açýklýk: | -7.4 |
| özdevim Yükselim: | -19.2 |
| B-T magnitude: | 6.238 |
| V-T magnitude: | 6.366 |
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