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Variable stars
Results: 220

#	Item
131	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 Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-02-01 05:00:28 Astrometry Space Physical cosmology Cepheid variable RR Lyrae variable Cosmic distance ladder Type II Cepheid Kepler Star Astronomy Standard candles Variable stars
132	Short Cadence Cepheid targets – K2 Campaign 0 E. Plachy1,2 , L. Moln´ar1,2 , R. Szab´o1 , P. A. Moskalik3 , L. Szabados1 , K. Kolenberg4 , N. R. Evans4 , C. C. Ngeow5 , R. Smolec3 , A. Derekas1 , K. Kinemuchi6 , and Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-02-01 05:10:17 Astrometry Space Physical cosmology Cepheid variables Classical Cepheid variable Cosmic distance ladder W Virginis variable Type II Cepheid Kepler Variable stars Astronomy Standard candles
133	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 Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-01-31 08:36:56 Universe Cepheus constellation Light sources Astrophysics Sun Star Variable star Stellar evolution Helioseismology Astronomy Stellar astronomy Space
134	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 Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-02-01 05:20:24 Standard candles Blazhko effect Variable stars Lyra constellation Exoplanetology Sergey Blazhko RR Lyrae Kepler Cosmic distance ladder Astronomy Space RR Lyrae variables
135	K2 Campaign 0 Proposal for Monitoring Cataclysmic Variables Paula Szkody & Zhibin Dai (U of Washington); Peter Garnavich (U of Notre Dame) The original Kepler field contains 27 previously known and/or subsequently discov Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-02-01 01:24:07 Binary stars Cataclysmic variable star Exoplanetology Kepler mission Dwarf nova Johannes Kepler Intermediate polar Kepler Paula Szkody Astronomy Spacecraft Space
136	Asteroseismology of Stars in Eclipsing-‐Binary Systems -‐ Selection of Targets for Kepler2, Field 0 -‐ Patrick Gaulme ([removed]), Thie Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-02-03 02:02:55 Star types Exoplanetology Space telescopes Kepler mission European Space Agency COROT Kepler Variable star Binary star Spacecraft Spaceflight Space
137	Hubblecast Episode 71: Visible echoes around RS Puppis 00:00 [Narrator] 1. Everyone has heard echoes — but have you ever seen one? Hubble has. By watching the variable star RS Puppis, Hubble Add to Reading List Source URL: www.spacetelescope.org Language: English - Date: 2013-12-16 08:21:19 Puppis constellation Cepheid variables Binary stars Astrometry Standard candles RS Puppis Light echo V838 Monocerotis Variable star Astronomy Space Universe
138	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 Add to Reading List Source URL: keplerscience.arc.nasa.gov Language: English - Date: 2014-05-14 17:08:39 Star types Universe Instability strip Cepheid variable Star Κ mechanism Delta Scuti variable Stellar pulsations Astronomy Variable stars Space
139	Pulsating Variable Stars and the H-R Diagram -10 SR Add to Reading List Source URL: chandra.harvard.edu - Date: 2012-08-10 17:42:18
140	Pulsating Variable Stars and the H-R Diagram[removed] Add to Reading List Source URL: chandra.harvard.edu - Date: 2012-08-10 17:43:49

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