Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Buckley, David A.H."'
Autor:
McPhate, Jason B., Siegmund, Oswald H.W., Welsh, Barry Y., Vallerga, John V., Buckley, David A.H., Gulbis, Amanda A.S., Brink, Janus D., Rogers, Doug
Publikováno v:
In Physics Procedia 2012 37:1453-1460
Autor:
Thomas, Jessymol K., Charles, Philip, Buckley, David A.H., Paice, John A, Kotze, Marissa M., Lasota, J.P, Potter, Stephen, Steiner, James F.
The black hole X-ray transient MAXI J1820 + 070 (= ASSASN-18ey) discovered in 2018 March was one of the optically brightest ever seen, which has resulted in very detailed optical outburst light curves being obtained. We combine them here with X-ray a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______348::913ebd1c9d982801f94525d5e85e1c37
https://eprints.soton.ac.uk/454211/
https://eprints.soton.ac.uk/454211/
Autor:
Buckley, David A.H.
Publikováno v:
In New Astronomy Reviews 2001 45(1):13-16
Autor:
Buckley, David A.H.
Publikováno v:
In New Astronomy Reviews 2000 44(1):63-68
Autor:
Buckley, David A.H., Potter, Stephen B., Meintjes, Pieter J., Marsh, Tom R., Gänsicke, Boris T.
Publikováno v:
Galaxies (2075-4434); Mar2018, Vol. 6 Issue 1, p14, 7p
Autor:
Redaelli, Maurício, Kepler, Souza Oliveira, Costa, Jose Eduardo da Silveira, Winget, Donald Earl, Handler, Gerald, Castanheira, Bárbara Garcia, Kanaan Neto, Antonio Nemer, Fraga, Luciano, Henrique, P., Giovannini Junior, Odilon, Provencal, Judith L., Shipman, Harry L., Dalessio, J., Thompson, S. E., Mullally, Fergal, Brewer, M. M., Childers, D., Oksala, M. E., Rosen, Rachel, Wood, Matthew A., Reed, M. D., Walter, B., Strickland, Willie, Chandler, Dean W., Watson, Todd K., Nather, R. Edward, Montgomery, Michael Houston, Bischoff-Kim, Agnès, Hansen, Carl J., Nitta, Atsuko, Kleinman, Scot James, Claver, C.F., Brown, Tim, Sullivan, Denis J., Kim, Seung-Lee, Chen, Wen-Ping, Yang, M., Shih, Chia-You, Zhang, X, Jiang, Xiaojun, Fu, Jianning Ning, Seetha, S., Ashoka, B.N., Marar, T.M. Krishnan, Baliyan, Kiran S., Vats, Hari Om, Chernyshev, A.V., Ibbetson, Peter A., Leibowitz, Elia M., Hemar, Shirley, Sergeev, A., Andreev, M., Janulis, Rimvydas, Meistas, Edmundas G., Moskalik, Pawel, Pajdosz, Gabriel, Baran, Andrzej, Winiarski, M., Zola, Staszek, Ogloza, Waldemar, Siwak, Michal, Bognár, Zsófia, Solheim, Jan-Eric, Sefako, R., Buckley, David A.H., O'Donoghue, Darragh, Nagel, Thorsten, Silvotti, Roberto, Bruni, I., Fremy, J. R., Vauclair, Gérard, Chevreton, Michel, Dolez, Noël, Pfeiffer, Ben, Barstow, Martin A., Creevey, o, Kawaler, Steven D., Clemens, J. Christopher
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
PG 1351+489 is one of the 20DBVs – pulsating helium-atmospherewhite dwarf stars – known and has the simplest power spectrum for this class of star, making it a good candidate to study cooling rates. We report accurate period determinations for th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::d03745808ee70215fb9b16872abad91c
Autor:
Vuille, F., O'Donoghue, Darragh, Buckley, David A.H., Massacand, C.N., Solheim, Jan-Eric, Bard, S., Vauclair, Gérard, Giovannini Junior, Odilon, Kepler, Souza Oliveira, Kanaan Neto, Antonio Nemer, Provencal, Judith L., Wood, Matthew A., Clemens, J. Christopher, Kleinman, Scot James, O'Brien, M. Sean, Nather, R. Edward, Winget, Donald Earl, Nitta, Atsuko, Klumpe, Eric W., Montgomery, Michael Houston, Watson, Todd K., Bradley, Paul A., Sullivan, Denis J., Wu, K., Marar, T.M. Krishnan, Seetha, S., Ashoka, B.N., Mahra, H.S., Bhat, B.C., Babu, V.C., Leibowitz, Elia M., Hemar, Shirley, Ibbetson, Peter A., Mashal, E., Meistas, Edmundas G., Moskalik, Pawel, Zola, Staszek, Krzesinski, Jerzy, Pajdosz, Gabriel
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
We present a detailed mode identification performed on the 1994 Whole Earth Telescope (WET) run on GD 358. The results are compared with that obtained for the same star from the 1990 WET data. The two temporal spectra show very few qualitative differ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::12cba0870b469004f6446770e8b602d2
Autor:
Handler, Gerald, Pikall, H., O'Donoghue, Darragh, Buckley, David A.H., Vauclair, Gérard, Chevreton, Michel, Giovannini Junior, Odilon, Kepler, Souza Oliveira, Goode, P.R., Provencal, Judith L., Wood, Matthew A., Clemens, J. Christopher, O'Brien, M. Sean, Nather, R. Edward, Winget, Donald Earl, Kleinman, Scot James, Kanaan Neto, Antonio Nemer, Watson, Todd K., Nitta, Atsuko, Montgomery, Michael Houston, Klumpe, Eric W., Bradley, Paul A., Sullivan, Denis J., Wu, K., Marar, T.M. Krishnan, Seetha, S., Ashoka, B.N., Mahra, H.S., Bhat, B.C., Babu, V.C., Leibowitz, Elia M., Hemar, Shirley, Ibbetson, Peter A., Mashal, E., Meistas, Edmundas G., Dziembowski, W.A., Pamyantnykh, A.A., Moskalik, Pawel, Zola, Staszek, Pajdosz, Gabriel, Krzesinski, Jerzy, Solheim, Jan-Eric, Bard, S., Massarand, C.M., Breger, M., Gelbmann, M.J., Paunzen, E., North, P.
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
92 h of new Whole Earth Telescope observations have been acquired for the δ Scuti star CD -24 7599. All the seven pulsation modes reported by Handler et al. are confirmed. However, significant amplitude variations which are not caused by beating of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::101cb14882b3e117e2e3a5c2bceb3839
Autor:
Handler, Gerald, Breger, M., Sullivan, Denis J., Peet, A.J. van der, Clemens, J. Christopher, O'Donoghue, Darragh, Chen, A.-L., Kanaan Neto, Antonio Nemer, Sterken, C., Claver, C.F., Krisciunas, K., Kleinman, Scot James, Wickramasinghe, D.T., Wills, Beverley J., Provencal, Judith L., Nather, R. Edward, Winget, Donald Earl, Watson, Todd K., Barstow, Martin A., Buckley, David A.H.
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
We report a frequency analysis of the δ Scuti star CD-24°7599 and the discovery that it pulsates nonradially with at least 7 frequencies between 27.01 and 38.11 cycles per day (312 to 441 μHz). These results are based on 116.7 hours of photometric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::47a755ec61e23ed45f9ff5f956dc9162
Autor:
Kepler, Souza Oliveira, Giovannini Junior, Odilon, Wood, Matthew A., Nather, R. Edward, Winget, Donald Earl, Kanaan Neto, Antonio Nemer, Kleinman, Scot James, Bradley, Paul A., Provencal, Judith L., Clemens, J. Christopher, Claver, C.F., Watson, Todd K., Yanagida, K., Krisciunas, K., Marar, T.M. Krishnan, Seetha, S., Ashoka, B.N., Leibowitz, Elia M., Mendelson, Haim, Mazeh, Tsevi, Moskalik, Pawel, Krzesinski, Jerzy, Pajdosz, Y., Zola, Staszek, Solheim, Jan-Eric, Emanuelsen, P.-I., Dolez, Noël, Vauclair, Gérard, Chevreton, Michel, Fremy, J. R., Barstow, Martin A., Sansom, A.E., Tweedy, R.W., Wickramasinghe, D.T., Ferrario, Lilia, Sullivan, Denis J., Peet, A.J. van der, Buckley, David A.H., Chen, A.-L.
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
We observed G226-29 for 121 hr in 1992 February and confirm the presence of the three previously identified frequencies close to 109 s. We find no evidence of other pulsation periods down to our noise level of about 0.35 millimodulation amplitudes. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::d7c66bcbcaaf26a7a293c8f88a00304d