LMC Cepheids radial velocities (Storm+, 2011)

Details LMC Cepheids radial velocities (Storm+, 2011) LMC Cepheids radial velocities (Storm+, 2011)

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35349095s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/534/A95. Originally published in: 2011A&A...534A..95S

Physics

Magellanic Clouds, Stars: Variable, Stars: Distances, Radial Velocities

Scientific paper

We present 509 high precision radial velocity measurements for a total of 22 LMC Cepheids obtained with the HARPS spectrograph at the ESO 3.6m telescope, and the FEROS spectrograph on the ESO/MPG 2.2m telescope both at La Silla, Chile. From these data radial velocity curves with good phase coverage can be established. The Cepheids have pulsational periods ranging from about 5 to 80 days. The Cepheids are: HV873, HV876, HV877, HV878, HV881, HV900, HV914, HV1005, HV1006, HV1023, HV2282, HV2369, HV2405, HV2527, HV2538, HV2549, HV5655, HV6093, HV12452, HV12505, HV12717, U1 (= EV* LMC V0033).
(2 data files).

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