Parents

Sign in to add mentor
Roger Alistair Bell grad student 1969 University of Maryland (Astronomy Tree)
 (Solar magnesium isotopic abundance ratios.)
BETA: Related publications

Publications

You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Friesen B, Baron E, Parrent JT, et al. (2017) Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times Monthly Notices of the Royal Astronomical Society. 467: 2392-2411
McCully C, Jha SW, Foley RJ, et al. (2014) Hubble space Telescope and ground-based observations of the Type Iax Supernovae SN 2005HK and SN 2008A Astrophysical Journal. 786
Friesen B, Baron E, Branch D, et al. (2012) Supernova resonance-scattering line profiles in the absence of a photosphere Astrophysical Journal, Supplement Series. 203
Branch D. (2010) Supernovae: New explosions of old stars? Nature. 465: 303-4
Branch D, Dang LC, Baron E. (2009) Comparative Direct Analysis of Type Ia Supernova Spectra. V. Insights from a Larger Sample and Quantitative Subclassification Publications of the Astronomical Society of the Pacific. 121: 238-247
Pastorello A, Mattila S, Zampieri L, et al. (2008) Massive stars exploding in a He-rich circumstellar medium - I. Type Ibn (SN 2006jc-like) events Monthly Notices of the Royal Astronomical Society. 389: 113-130
Bongard S, Baron E, Smadja G, et al. (2008) Multilayered spectral formation in type Ia supenovae around maximum light Astrophysical Journal. 687: 456-465
Clocchiatti A, Wheeler JC, Kirshner RP, et al. (2008) Late-time HST photometry of SN 1994I: Hints of positron annihilation energy deposition Publications of the Astronomical Society of the Pacific. 120: 290-300
Casebeer D, Baron E, Leighly K, et al. (2008) A self-consistent NLTE-spectra synthesis model of FeLoBAL QSOs Astrophysical Journal. 676: 857-867
Branch D, Jeffery DJ, Parrent J, et al. (2008) Comparative Direct Analysis of Type Ia Supernova Spectra. IV. Postmaximum Publications of the Astronomical Society of the Pacific. 120: 135-149
See more...