KASC

Results: 49



#Item
31Long Cadence Cepheid targets – K2 Campaign 0 L. Moln´ar1,2 , R. Szab´o1 , P. A. Moskalik3 , E. Plachy1,2 , L. Szabados1 , K. Kolenberg4 , N. R. Evans4 , C. C. Ngeow5 , A. Derekas1 , R. Smolec3 and the KASC RR Lyrae-C

Long Cadence Cepheid targets – K2 Campaign 0 L. Moln´ar1,2 , R. Szab´o1 , P. A. Moskalik3 , E. Plachy1,2 , L. Szabados1 , K. Kolenberg4 , N. R. Evans4 , C. C. Ngeow5 , A. Derekas1 , R. Smolec3 and the KASC RR Lyrae-C

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2014-02-01 05:00:28
32K2 Proposal on behalf of KASC WG3  Asteroseismology and rotation of Am stars Prepared by L.A. Balona, G. Catanzaro and V. Ripepi In Am stars the metal lines indicate a later spectral type than that derived from the Balme

K2 Proposal on behalf of KASC WG3 Asteroseismology and rotation of Am stars Prepared by L.A. Balona, G. Catanzaro and V. Ripepi In Am stars the metal lines indicate a later spectral type than that derived from the Balme

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Language: English - Date: 2014-01-31 08:34:10
33K2 Proposal on behalf of KASC WG3  Asteroseismology and rotation of Be stars Prepared by Luis Balona & Juan Fabregat The Be stars are normal B stars which show emission, or partial emission, in one or more Balmer lines.

K2 Proposal on behalf of KASC WG3 Asteroseismology and rotation of Be stars Prepared by Luis Balona & Juan Fabregat The Be stars are normal B stars which show emission, or partial emission, in one or more Balmer lines.

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Language: English - Date: 2014-01-31 08:37:11
34K2 Proposal on behalf of KASC WG3  Asteroseismology of Beta Cephei stars Prepared by Luis Balona, Gerald Handler and Peter De Cat Even nowadays, the interior structure of main sequence stars and their temporal evolution

K2 Proposal on behalf of KASC WG3 Asteroseismology of Beta Cephei stars Prepared by Luis Balona, Gerald Handler and Peter De Cat Even nowadays, the interior structure of main sequence stars and their temporal evolution

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2014-01-31 08:36:56
35Long cadence RR Lyrae targets - K2 Mission / C0 campaign R. Szabó1, E. Plachy1,2, K. Kolenberg3, L. Molnár1,2, E. Guggenberger4, J. M. Benkő1, P. Moskalik5, J. Nemec6, C-C. Ngeow7+ KASC WG#7 1 Konkoly Observatory, Hun

Long cadence RR Lyrae targets - K2 Mission / C0 campaign R. Szabó1, E. Plachy1,2, K. Kolenberg3, L. Molnár1,2, E. Guggenberger4, J. M. Benkő1, P. Moskalik5, J. Nemec6, C-C. Ngeow7+ KASC WG#7 1 Konkoly Observatory, Hun

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Language: English - Date: 2014-02-01 05:20:24
36K2 Proposal on behalf of KASC WG3  Asteroseismology of SPB stars Prepared by Peter De Cat, Gerald Handler, Louis Balona, Victoria Antoci & Jan Cuypers Slowly pulsating B (SPB) stars are mid-to-late B-type stars in the ma

K2 Proposal on behalf of KASC WG3 Asteroseismology of SPB stars Prepared by Peter De Cat, Gerald Handler, Louis Balona, Victoria Antoci & Jan Cuypers Slowly pulsating B (SPB) stars are mid-to-late B-type stars in the ma

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2014-01-31 08:35:57
37Asteroseismology of bright Red Giants KASC Working Group 8: K2 field 1 Target Proposal Point of Contact: Víctor Silva Aguirre ([removed]) Abstract We propose to observe a small number of bright nearby red giant

Asteroseismology of bright Red Giants KASC Working Group 8: K2 field 1 Target Proposal Point of Contact: Víctor Silva Aguirre ([removed]) Abstract We propose to observe a small number of bright nearby red giant

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Language: English - Date: 2014-05-14 17:08:40
38Solar-Type Stars for Asteroseismology in K2 Short Cadence KASC Working Group 1: K2 Field 1 Target Proposal (Point of contact: Bill Chaplin, [removed]) Science Case: This document proposes a selection of very

Solar-Type Stars for Asteroseismology in K2 Short Cadence KASC Working Group 1: K2 Field 1 Target Proposal (Point of contact: Bill Chaplin, [removed]) Science Case: This document proposes a selection of very

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Language: English - Date: 2014-05-14 17:08:40
39A survey to detect first sdB Planetary Transits R. Silvotti (INAF-OATo), R.H. Østensen (KU Leuven) and the KASC WG11 Although only 2% of stars evolve through the subdwarf B (sdB) phase (Heber 1986, A&A 155, 33; see Hebe

A survey to detect first sdB Planetary Transits R. Silvotti (INAF-OATo), R.H. Østensen (KU Leuven) and the KASC WG11 Although only 2% of stars evolve through the subdwarf B (sdB) phase (Heber 1986, A&A 155, 33; see Hebe

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2014-05-14 17:08:40
40Pulsations and the Am Stars Barry Smalley (Keele University) on behalf of KASC WG 3 In the region of the HR Diagram where the Cepheid instability strip extends across the main sequence, there is a complex relationship be

Pulsations and the Am Stars Barry Smalley (Keele University) on behalf of KASC WG 3 In the region of the HR Diagram where the Cepheid instability strip extends across the main sequence, there is a complex relationship be

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Language: English - Date: 2014-05-14 17:08:39