Výsledky vyhledávání - "Healy, A. M."

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Discovery of a nova super-remnant cavity surrounding RS Ophiuchi

Autor: Healy-Kalesh, M. W., Darnley, M. J., Harvey, E. J., Newsam, A. M.

The prototypical nova super-remnant (NSR) was uncovered around the most rapidly recurring nova (RN), M31N 2008-12a. Simulations of the growth of NSRs revealed that these large structures should exist around all novae, whether classical or recurrent.

Externí odkaz: http://arxiv.org/abs/2402.05855

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On an apparent dearth of recurrent nova super-remnants in the Local Group

Autor: Healy-Kalesh, M. W., Darnley, M. J., Shara, M. M.

The Andromeda Galaxy is home to the annually erupting recurrent nova (RN) M31N 2008-12a (12a); the first nova found to host a nova super-remnant (NSR). A NSR is an immense structure surrounding a RN, created from many millions of eruptions sweeping u

Externí odkaz: http://arxiv.org/abs/2401.04583

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Hydrodynamic simulations of the KT Eridani nova super-remnant

Autor: Healy-Kalesh, M. W., Darnley, M. J., Shara, M. M., Lanzetta, K. M., Garland, J. T., Gromoll, S.

A nova super-remnant (NSR) is an immense structure associated with a nova that forms when frequent and recurrent nova eruptions sweep up surrounding interstellar material (ISM) into a high density and distant shell. The prototypical NSR, measuring ov

Externí odkaz: http://arxiv.org/abs/2310.17258

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On the Observability of Recurrent Nova Super-Remnants

Autor: Healy-Kalesh, M. W., Darnley, M. J., Harvey, E. J., Copperwheat, C. M., James, P. A., Andersson, T., Henze, M., O'Brien, T. J.

The nova super-remnant (NSR) surrounding M31N 2008-12a (12a), the annually erupting recurrent nova (RN), is the only known example of this phenomenon. As this structure has grown as a result of frequent eruptions from 12a, we might expect to see NSRs

Externí odkaz: http://arxiv.org/abs/2302.11900

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