Search Results - "Strawn, Emily"

Changes in the Na D1 Absorption Components of η Carinae Provide Clues on the Location of the Dissipating Central Occulter by Pickett, Connor S., Richardson, Noel D., Gull, Theodore R., Hillier, D. John, Hartman, Henrik, Ibrahim, Nour, Lane, Alexis M., Strawn, Emily, Damineli, Augusto, Moffat, Anthony F. J., Navarete, Felipe, Weigelt, Gerd

“…The Na D absorption doublet in the spectrum of η Carinae is complex, with multiple absorption features associated with the Great Eruption (1840s), the Lesser…”
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The orbital kinematics of η Carinae over three periastra with a possible detection of the elusive secondary’s motion by Strawn, Emily, Richardson, Noel D, Moffat, Anthony F J, Ibrahim, Nour, Lane, Alexis, Pickett, Connor, Chené, André-Nicolas, Corcoran, Michael F, Damineli, Augusto, Gull, Theodore R, Hillier, D John, Morris, Patrick, Pablo, Herbert, Thomas, Joshua D, Stevens, Ian R, Teodoro, Mairan, Weigelt, Gerd

“…ABSTRACT The binary η Carinae is the closest example of a very massive star, which may have formed through a merger during its Great Eruption in the mid-19th…”
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Changes in the Na D$_1$ Absorption Components of $\eta$ Carinae Provide Clues on the Location of the Dissipating Central Occulter by Pickett, Connor S, Richardson, Noel D, Gull, Theodore, Hillier, D. John, Hartman, Henrik, Ibrahim, Nour, Lane, Alexis M, Strawn, Emily, Damineli, Augusto, Moffat, Anthony F. J, Navarete, Felipe, Weigelt, Gerd

“…The Na D absorption doublet in the spectrum of $\eta$ Carinae is complex, with multiple absorption features associated with the Great Eruption (1840s), the…”
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The orbital kinematics of eta Carinae over three periastra with a possible detection of the elusive secondary's motion by Strawn, Emily, Richardson, Noel D, Moffat, Anthony F. J, Ibrahim, Nour, Lane, Alexis, Pickett, Connor, Chené, André-Nicolas, Corcoran, Michael F, Damineli, Augusto, Gull, Theodore R, Hillier, D. John, Morris, Patrick, Pablo, Herbert, Thomas, Joshua D, Stevens, Ian R, Teodoro, Mairan, Weigelt, Gerd

“…The binary eta Carinae is the closest example of a very massive star, which may have formed through a merger during its Great Eruption in the mid-nineteenth…”
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