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pro vyhledávání: '"variables: T Tauri [Stars]"'
Akademický článek
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Autor:
Bischoff, R., Raetz, St, Fernández, Matilde, Mugrauer, M., Neuhäuser, R., Huang, P. C., Chen, W. P., Sota Ballano, Alfredo, Jiménez Ortega, Jaime, Hambaryan, V. V., Zieliński, P., Dróżdż, M., Ogłoza, W., Stenglein, W., Hohmann, E., Michel, K. -U.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The T Tauri star CVSO 30, also known as PTFO 8-8695, was studied intensively with ground-based telescopes as well as with satellites over the last decade. It showed a variable light curve with additional repeating planetary transit-like dips every
Publikováno v:
Open Astronomy
The dynamics of magnetic flux tubes (MFTs) in the accretion disk of typical Herbig Ae/Be star with fossil large-scale magnetic field is modeled taking into account the buoyant and drag forces, radiative heat exchange with the surrounding gas, and the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69965eed49b6038e256a30a7702b9aec
Autor:
Alejandra Traspas Munia, Igor Kudzej, Geoffrey Stone, Mark C. Price, P. Mikołajczyk, S. J. Billington, Barry Merrikin, Alfred Kume, Carys Herbert, Mario Morales Aimar, Esteban Fernández Mañanes, Steve Rau, Timothy P. Long, Tarik Zegmott, Franky Dubois, Bringfried Stecklum, Tim Nelson, Tonny Vanmunster, George Fleming, Efthymia Derezea, Nick Quinn, Rafael Gonzalez Farfán, Krzysztof Kotysz, Klaas Wiersema, Rafael Castillo García, Francisco C. Soldán Alfaro, Georg Piehler, Domenico Licchelli, Mark M. Phillips, Jochen Eislöffel, Jack J. Evitts, T. Killestein, Heinz-Bernd Eggenstein, Michael A. Heald, Diego Rodríguez, Pavol A. Dubovský, Thomas Urtly, Marc Deldem, Erik Schwendeman, D. Moździerski, Aleks Scholz, Katarzyna Kowalska, Siegfried Vanaverbeke, J. Campbell-White, Niall Miller, Ludwig Logie, Dirk Froebrich, S. V. Makin, Roger D. Pickard, Lord Dover, Stephen R. L. Futcher, Tony Vale, Stephen Johnstone
Studying rotational variability of young stars is enabling us to investigate a multitude of properties of young star-disk systems. We utilise high cadence, multi-wavelength optical time series data from the Hunting Outbursting Young Stars citizen sci
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::307f9345f22fe82de46de2cc5f9a1929
https://hdl.handle.net/10023/24057
https://hdl.handle.net/10023/24057
Autor:
Enrique Solano, I. Mendigutía, P. Marcos-Arenal, J. Guzmán-Díaz, M. Vioque, Carlos Rodrigo, Gwendolyn Meeus, Rene D. Oudmaijer, Benjamin Montesinos
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
instname
(Abridged) Herbig Ae/Be stars (HAeBes) have so far been studied based on relatively small samples that are scattered throughout the sky. Their fundamental stellar and circumstellar parameters and statistical properties were derived with heterogeneous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9429ab3f8330aa06a4a6a34257995114
https://eprints.whiterose.ac.uk/176427/1/2104.11759.pdf
https://eprints.whiterose.ac.uk/176427/1/2104.11759.pdf
Autor:
Petrov, P. P., Romanova, M. M., Grankin, K. N., Artemenko, S. A., Babina, E. V., Yu Gorda, S.
Publikováno v:
Mon. Not. R. Astron. Soc.
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
Planets are thought to form at the early stage of stellar evolution when mass accretion is still ongoing. RY Tau is a T Tauri type star at the age of a few Myr, with an accretion disc seen at high inclination, so that the line of sight crosses both t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______917::1ff805e31abb528e1dc1e3ef2e1e0df9
https://hdl.handle.net/10995/111387
https://hdl.handle.net/10995/111387
Autor:
Filocomo, Agostina, Escobar, Gastón J., Albacete Colombo, Juan Facundo, Pássaro, Emiliano A., Combi, Jorge A.
Publikováno v:
RID-UNRN (UNRN)
Universidad Nacional de Río Negro
instacron:UNRN
Universidad Nacional de Río Negro
instacron:UNRN
Fil: Albacete Colombo, Juan F. Universidad Nacional de Río Negro. Río Negro, Argentina. Fil: Filocomo, Agostina. Universidad Nacional de Río Negro. Río Negro, Argentina. Fil: Filocomo, Agostina. Instituto Argentino de Radioastronomía, CONICET–
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::832a56d93f653ba04e467d423d3820f0
http://rid.unrn.edu.ar/handle/20.500.12049/5390
http://rid.unrn.edu.ar/handle/20.500.12049/5390
Autor:
D. Baines, I. Mendigutía, Nami Mowlavi, M. Vioque, Ricardo Pérez-Martínez, Rene D. Oudmaijer, M. Schreiner
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
The intermediate-mass pre-main sequence Herbig Ae/Be stars are key to understanding the differences in formation mechanisms between low- and high-mass stars. The study of the general properties of these objects is hampered by the fact that few and mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0697244e9ead48fdbed5af655563ca1
http://arxiv.org/abs/2005.01727
http://arxiv.org/abs/2005.01727
Autor:
Peña, Carlos Contreras, Johnstone, Doug, Baek, Giseon, Herczeg, Gregory J., Mairs, Steve, Scholz, Aleks, Lee, Jeong-Eun, Team, The JCMT Transient
We study the relationship between the mid-infrared and sub-mm variability of deeply embedded protostars using the multi-epoch data from the Wide Infrared Survey Explorer ($WISE$/NEOWISE) and the ongoing James Clerk Maxwell Telescope (JCMT) transient
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61b8f93f52a0bff12f2a26d001f9c32e
http://arxiv.org/abs/2005.01569
http://arxiv.org/abs/2005.01569
Autor:
C. Wichittanakom, I. Mendigutía, K. M. Ababakr, Miguel Vioque, Rene D. Oudmaijer, J. R. Fairlamb
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
This work presents a spectroscopic study of 163 Herbig Ae/Be stars. Amongst these, we present new data for 30 objects. Stellar parameters such as temperature, reddening, mass, luminosity, and age are homogeneously determined. Mass accretion rates are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c45585c2558b8c5f1995cc297bab3a2e
http://hdl.handle.net/10261/234198
http://hdl.handle.net/10261/234198