Zobrazeno 1 - 10
of 57
pro vyhledávání: '"Weidmann, W. A."'
Autor:
Weidmann, W. A., Mari, M. B., Schmidt, E. O., Gaspar, G., Bertolami, M. M. Miller, Oio, A. G., Gutiérrez-Soto, L. A., Volpe, M. G., Gamen, R., Mast, D.
Publikováno v:
A&A 640, A10 (2020)
Planetary nebulae represent a potential late stage of stellar evolution, however the central stars (CSPNe) are relatively faint and therefore pertinent information is merely available for <20% of the Galactic sample. Consequently, the literature was
Externí odkaz:
http://arxiv.org/abs/2005.10368
Akademický článek
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Autor:
Weidmann, W., Gamen, R., Mast, D., Fariña, C., Gimeno, G., Schmidt, E. O., Ashley, R. P., de Arriba, L. Peralta, Sowicka, P., Ordonez-Etxeberria, I.
Publikováno v:
A&A 614, A135 (2018)
Context. There are more than 3000 known Galactic planetary nebulae (PNe), but only 492 central stars of Galactic planetary nebulae (CSPN) have known spectral types. It is vital to increase this number in order to have reliable statistics, which will
Externí odkaz:
http://arxiv.org/abs/1802.02122
Autor:
Weidmann, W. A., Schmidt, E. O., Valdarenas, R. R. Vena, Ahumada, J. A., Volpe, M. G., Mudrik, A.
We present an atlas of more than one hundred original images of planetary nebulae (PNe). These images were taken in a narrow-band filter centred on the nebular emission of the [N II] during several observing campaigns using two moderate-aperture tele
Externí odkaz:
http://arxiv.org/abs/1606.01066
Akademický článek
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Be objects are stars of B spectral type showing lines of the Balmer series in emission. The presence of these lines is attributed to the existence of an extended envelope, disk type, around them. Some stars are observed in both the Be and normal B-ty
Externí odkaz:
http://arxiv.org/abs/1305.7098
We perform a multiwavelength study toward the SNR G18.1-0.1 and nearby several HII regions (infrared dust bubbles N21 and N22, and the HII regions G018.149-00.283 and G18.197-00.181). Our goal is to provide observational evidence supporting that mass
Externí odkaz:
http://arxiv.org/abs/1305.2354
Planetary nebulae (PNe) are powerful tracers of evolved stellar populations. Among the 3000 known PNe in the Galaxy, about 600 are located within the 520 square-degree area covered by the VVV survey. The VVV photometric catalogue provides an importan
Externí odkaz:
http://arxiv.org/abs/1304.3755
Autor:
Saito, R. K., Hempel, M., Minniti, D., Lucas, P. W., Rejkuba, M., Toledo, I., Gonzalez, O. A., Alonso-Garcia, J., Irwin, M. J., Gonzalez-Solares, E., Hodgkin, S. T., Lewis, J. R., Cross, N., Ivanov, V. D., Kerins, E., Emerson, J. P., Soto, M., Amores, E. B., Gurovich, S., Dekany, I., Angeloni, R., Beamin, J. C., Catelan, M., Padilla, N., Zoccali, M., Pietrukowicz, P., Bidin, C. Moni, Mauro, F., Geisler, D., Folkes, S. L., Sale, S. E., Borissova, J., Kurtev, R., Ahumada, A. V., Alonso, M. V., Adamson, A., Arias, J. I., Bandyopadhyay, R. M., Barba, R. H., Barbuy, B., Baume, G. L., Bedin, L. R., Bellini, A., Benjamin, R., Bica, E., Bonatto, C., Bronfman, L., Carraro, G., Chene, A. N., Claria, J. J., Clarke, J. R. A., Contreras, C., Corvillon, A., de Grijs, R., Dias, B., Drew, J. E., Farina, C., Feinstein, C., Fernandez-Lajus, E., Gamen, R. C., Gieren, W., Goldman, B., Gonzalez-Fernandez, C., Grand, R. J. J., Gunthardt, G., Hambly, N. C., Hanson, M. M., Helminiak, K. G., Hoare, M. G., Huckvale, L., Jordan, A., Kinemuchi, K., Longmore, A., Lopez-Corredoira, M., Maccarone, T., Majaess, D., Martin, E. L., Masetti, N., Mennickent, R. E., Mirabel, I. F., Monaco, L., Morelli, L., Motta, V., Palma, T., Parisi, M. C., Parker, Q., Penaloza, F., Pietrzynski, G., Pignata, G., Popescu, B., Read, M. A., Rojas, A., Roman-Lopes, A., Ruiz, M. T., Saviane, I., Schreiber, M. R., Schroder, A. C., Sharma, S., Smith, M. D., Sodre Jr., L., Stead, J., Stephens, A. W., Tamura, M., Tappert, C., Thompson, M. A., Valenti, E., Vanzi, L., Walton, N. A., Weidmann, W., Zijlstra, A.
The ESO Public Survey VISTA Variables in the Via Lactea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for ~5 years. In this paper we describe the progress of the survey observ
Externí odkaz:
http://arxiv.org/abs/1111.5511
context About 2500 planetary nebulae are known in our Galaxy but only 224 have central stars with reported spectral types in the Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker et al. 1992; Acker et al. 1996) % aims We have started an o
Externí odkaz:
http://arxiv.org/abs/0806.4968