Studying circumstellar envelopes with ALMA David Neufeld Johns Hopkins University.
IR Shell Surrounding the Pulsar Wind Nebula G54.1+0.3 SNRs and PWNe in the Chandra Era Boston, July 8, 2009 Tea Temim (CfA, Univ. of MN) Collaborators:
Spectrographs. Literature: Astronomical Optics, Daniel Schroeder Astronomical Observations, Gordon Walker Stellar Photospheres, David Gray.
Studying circumstellar envelopes with ALMA
Within-Season Changes in the Periods and Light Curves of W UMa Binaries Russ Genet Orion Observatory Tom Smith Dark Ridge Observatory Dirk Terrell Southwest.
Within-Season Changes in the Periods and Light Curves of W UMa Binaries
Using the GR model Some important remarks * Danezis E., *Lyratzi E, *Antoniou A., **Popović L. Č., **Dimitriević M. S. *University of Athens, School of.
Observational signatures for shocks in the solar photosphere – possible HINODE/SOT observations
Variability of Be Stars: A Key to the Structure of their Circumstellar Environments Anatoly Miroshnichenko University of Toledo Variable Star Meeting 2004.
Spectrographs. Spectral Resolution d 1 2 Consider two monochromatic beams They will just be resolved when they have a wavelength separation of d Resolving.
Spectrographs. Literature: Astronomical Optics, Daniel Schneider Astronomical Observations, Gordon Walker Stellar Photospheres, David Gray.
The Z A strophysical P lasma P roperties ( ZAPP ) Collaboration
