1 / 10

HR 7355 and HR 5907: The MOST rapidly-rotating magnetic stars

HR 7355 and HR 5907: The MOST rapidly-rotating magnetic stars. Gregg Wade (RMC) on behalf of the MiMeS Collaboration. The MiMeS Project Magnetism in Massive Stars. Discovering the most rapidly rotating magnetic star(s).

Download Presentation

HR 7355 and HR 5907: The MOST rapidly-rotating magnetic stars

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. HR 7355 and HR 5907: The MOST rapidly-rotating magnetic stars • Gregg Wade (RMC) • on behalf of the MiMeS Collaboration

  2. The MiMeSProject Magnetism in Massive Stars

  3. Discovering the most rapidly rotating magnetic star(s) • Before MiMeS the B2Ve He-strong star HD 37017 fastest rotating magnetic massive star • P~0.9 d • MiMeS discovers most rapidly rotating magnetic star Sept/09 (HR 7355, Oksala et al. 2010) • P= 0.521 4404 d <- Based on HIPPARCOS/CTIO • Feb/10 – MiMeS discovers a nearly-identical rapidly rotating magnetic star (HR 5907, B2V) • P=0.50830 d -> NEW RECORD HOLDER!!

  4. HR 7355 - B2Ve P=0.5214404 d

  5. HR 5907 - B2Ve

  6. Rotationally-supported magnetospheres

  7. Doppler Imaging He I

  8. Significance of these results • Extreme testbeds • Near twins • Timescales and mechanisms for magnetic braking • Magnetospheric structure, density, emissivity • Role of rapid rotation and field geometry in channeling and confining winds of massive stars • Link to Be stars: Keplerian vs. rigid discs • Role of slow rotation in generating photospheric chemical peculiarities

  9. MOST observations ofHR 7355 and HR 5907 • High precision lightcurves are a vital complement to spectroscopic and polarimetric monitoring: • Confirm and refine rotational periods • Test limits of RRM model in ultra-rapid rotation regime • Constrain magnetospheric geometry and density • Disentangle magnetospheric vs spot contributions • Provide baseline for direct spindown measurement • Technical requirements: • 1 mmag errors, 1% (?) phase sampling (7 min integrations) • Acquired over multiple subsequent cycles or continuously

  10. Parameters ofHR 7355 and HR 5907 • HR 7355 • RA 19h24 • Dec -28 deg • V = 6.0 • Prot = 0.5214404 d • HR 5907 • RA 15h53 • Dec -24 deg • V = 5.4 • Prot = 0.50283 d

More Related