New publication based on ARAS spectra: MWC560 in 2016
Posted: Wed May 08, 2019 8:09 am
A new paper has been published by A. Lucy & al.
Regulation of accretion by its outflow in a symbiotic star: the 2016 outflow fast state of MWC 560
https://arxiv.org/pdf/1905.02399.pdf
It includes our colleagues Peter Somogyi and Umberto Sollecchia as co-authors.
and uses many spectra from ARAS database.
We are similarly indebted to all the other AAVSO, ARAS, and independent observers across the world whose work made this paper possible: H. Adler, S. Aguirre, T. Atwood, D. Barrett, P. Berardi, B. Billiaert, D. Blane, E. Blown, J. Bortle, D. Boyd, J. Briol, C. Buil, F. Campos, A. Capetillo Blanco, R. Carstens, J. Castellani, W. Clark, T. Colombo, A. Debackere, X. Domingo Martinez, S. Dvorak, J. Edlin, J. Foster, R. Fournier, L. Franco, J. Garlitz, A. Garofide, A. Glez-Herrera, K. Graham, C. Gualdoni, J. Guarro Flo, J. Foster, F. Guenther, C. Hadhazi, F. Hambsch, B. Harris, D. Jakubek, P. Lake, T. Lester, S. Lowther, C. Maloney, H. Matsuyama, K. Menzies, V. Mihai, J. Montier, G. Murawski, E. Muyllaert, G. Myers, P. Nelson, M. Nicholas, O. Nickel, S. O’Connor, J. O’Neill, W. Parentals, A. Plummer, G. Poyner, S. Richard, J. Ripero Osorio, J. Ritzel, D. Rodriguez Perez, R. Sabo, L. Shotter, P. Steffey, W. Strickland, D. Suessman, F. Teyssier, T. Vale, P. Vedrenne, A. Wargin, and A. Wilson. Many of these observers’ data were reproduced in Fig. 1. We apologize to any observers we neglected to acknowledge, with deep gratitude. We thank the staff of the AAVSO International Database and the ARAS Spectral Data Base, including E. Waagen and F. Teyssier.
Note: the current state of V694 Mon is very intertesting: high luminosity and desappearance of the strong high velocities absorptions. Observations of V694 Mon asap in september are strongly exhorted.
François Teyssier
Regulation of accretion by its outflow in a symbiotic star: the 2016 outflow fast state of MWC 560
https://arxiv.org/pdf/1905.02399.pdf
It includes our colleagues Peter Somogyi and Umberto Sollecchia as co-authors.
and uses many spectra from ARAS database.
We are similarly indebted to all the other AAVSO, ARAS, and independent observers across the world whose work made this paper possible: H. Adler, S. Aguirre, T. Atwood, D. Barrett, P. Berardi, B. Billiaert, D. Blane, E. Blown, J. Bortle, D. Boyd, J. Briol, C. Buil, F. Campos, A. Capetillo Blanco, R. Carstens, J. Castellani, W. Clark, T. Colombo, A. Debackere, X. Domingo Martinez, S. Dvorak, J. Edlin, J. Foster, R. Fournier, L. Franco, J. Garlitz, A. Garofide, A. Glez-Herrera, K. Graham, C. Gualdoni, J. Guarro Flo, J. Foster, F. Guenther, C. Hadhazi, F. Hambsch, B. Harris, D. Jakubek, P. Lake, T. Lester, S. Lowther, C. Maloney, H. Matsuyama, K. Menzies, V. Mihai, J. Montier, G. Murawski, E. Muyllaert, G. Myers, P. Nelson, M. Nicholas, O. Nickel, S. O’Connor, J. O’Neill, W. Parentals, A. Plummer, G. Poyner, S. Richard, J. Ripero Osorio, J. Ritzel, D. Rodriguez Perez, R. Sabo, L. Shotter, P. Steffey, W. Strickland, D. Suessman, F. Teyssier, T. Vale, P. Vedrenne, A. Wargin, and A. Wilson. Many of these observers’ data were reproduced in Fig. 1. We apologize to any observers we neglected to acknowledge, with deep gratitude. We thank the staff of the AAVSO International Database and the ARAS Spectral Data Base, including E. Waagen and F. Teyssier.
Note: the current state of V694 Mon is very intertesting: high luminosity and desappearance of the strong high velocities absorptions. Observations of V694 Mon asap in september are strongly exhorted.
François Teyssier