IGAPS: the merged IPHAS and UVEX optical surveys of theNorthern Galactic Plane

Autor: M. Monguió, R. Greimel, J. E. Drew, G. Barentsen, P. J. Groot, M. J. Irwin, J. Casares, B. T. Gänsicke, P. J. Carter, J. M. Corral-Santana, N. P. Gentile-Fusillo, S. Greiss, L. M. van Haaften, M. Hollands, D. Jones, T. Kupfer, C. J. Manser, D. N. A. Murphy, A. F. McLeod, T. Oosting, Q. A. Parker, S. Pyrzas, P. Rodríguez-Gil, J. van Roestel, S. Scaringi, P. Schellart, O. Toloza, O. Vaduvescu, L. van Spaandonk, K. Verbeek, N. J. Wright, J. Eislöffel, J. Fabregat, A. Harris, R. A. H. Morris, S. Phillipps, R. Raddi, L. Sabin, Y. Unruh, J. S. Vink, R. Wesson, A. Cardwell, A. de Burgos, R. K. Cochrane, S. Doostmohammadi, T. Mocnik, H. Stoev, L. Suárez-Andrés, V. Tudor, T. G. Wilson, T. J. Zegmott

Publikováno v: Astronomy & Astrophysics, 638, 1-26
Astronomy & Astrophysics
2020, ' IGAPS: the merged IPHAS and UVEX optical surveys of the northern Galactic plane ', Astronomy and Astrophysics, vol. 638 . https://doi.org/10.1051/0004-6361/201937333
Astronomy & Astrophysics, 638, pp. 1-26
2020, ' IGAPS : The merged IPHAS and UVEX optical surveys of the Northern Galactic Plane ', Astronomy and Astrophysics, vol. 638, A18 . https://doi.org/10.1051/0004-6361/201937333

The INT Galactic Plane Survey (IGAPS) is the merger of the optical photometric surveys, IPHAS and UVEX, based on data from the Isaac Newton Telescope (INT) obtained between 2003 and 2018. Here, we present the IGAPS point source catalogue. It contains

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7c56436e1a2ab4a2518123d7ec5a74e
http://arxiv.org/abs/2002.05157

Late-time evolution of ultracompact X-ray binaries

Autor: Gijs Nelemans, R. Voss, L. M. van Haaften

Publikováno v: Proceedings of the International Astronomical Union, 290, 153-156
Proceedings of the International Astronomical Union, 290, Symposium S290, pp. 153-156

Ultracompact X-ray binaries (UCXBs) have orbital periods shorter than about 80 minutes and typically consist of a neutron star that accretes hydrogen-poor matter from a white dwarf companion. Angular momentum loss via gravitational wave radiation dri

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2155106301992bb75a39426cf0cc27af
https://doi.org/10.1017/s1743921312019424

Population synthesis of ultracompact X-ray binaries in the Galactic bulge*

Autor: Silvia Toonen, Gijs Nelemans, L. R. Yungelson, R. Voss, S. Portegies Zwart, M. V. van der Sluys, L. M. van Haaften

Publikováno v: Astronomy & Astrophysics, 552, pp. A69(1)-A69(16)
Astronomy & Astrophysics, 552, A69(1)-A69(16)
Astronomy & Astrophysics, 552, A69

[abridged] Aims. We model the number and properties of ultracompact X-ray binaries (UCXBs) in the Galactic Bulge. The objective is to learn about the formation of UCXBs and their evolution, such as the onset of mass transfer and late-time behavior. M

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::643d47ff0ca93a89ddd302aba6d051d1
https://hdl.handle.net/https://repository.ubn.ru.nl/handle/2066/111213

Initial data release of the Kepler-INT Survey

Autor: Martin Still, Janet E. Drew, Peter G. Jonker, Simone Scaringi, Mike Irwin, L. M. van Haaften, Eric Martin, Vincenzo Ripepi, Nicholas J. Wright, Sandra Greiss, K. Verbeek, Boris T. Gänsicke, Jeremy J. Drake, Eduardo Gonzalez-Solares, John Southworth, Robert Greimel, Paul J. Groot, Danny Steeghs, Roy Ostensen, Christian Knigge, Sweta Shah, H. J. Farnhill

Publikováno v: The Astrophysical Journal, 144, 24
The Astronomical Journal
The Astrophysical Journal, 144, 1, pp. 24

This paper describes the first data release of the Kepler-INT Survey (KIS), that covers a 116 deg2 region of the Cygnus and Lyra constellations. The Kepler field is the target of the most intensive search for transiting planets to date. Despite the f

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53dbf5e12642738b6cc9e67d2a333c29

Long-term luminosity behavior of 14 ultracompact X-ray binaries

Autor: R. Voss, Gijs Nelemans, L. M. van Haaften

Publikováno v: Astronomy & Astrophysics, 543, pp. A121
Astronomy & Astrophysics, 543, A121

Context. X-ray binaries are usually divided in persistent and transient sources. For ultracompact X-ray binaries (UCXBs), the mass transfer rate is expected to be a strong function of orbital period, predicting persistent sources at short periods and

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8cab8dfaf132834626cced44babd751c
https://doi.org/10.1051/0004-6361/201118067