@article{MTMT:32706782,
	title = {Herschel/HIFI Discoveryof a Far-Infrared DIB Analog † ‡},
	url = {https://m2.mtmt.hu/api/publication/32706782},
	author = {Müller, H. S. P. and Schilke, P. and Gerin, M. and Lis, D. C. and Bergin, E. A. and Pearson, J. C. and De, Luca M. and Black, J. H.},
	doi = {10.1017/S1743921313015846},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {297},
	unique-id = {32706782},
	issn = {0074-1809},
	abstract = {The Herschel Space Observatory carried out observations at far-infrared wavelengths, which significantly increased our knowledge of the interstellar medium and the star-formation process in the Milky Way and external galaxies, as well as our understanding of astrochemistry. Absorption features, known, e.g., from observations at millimeter wavelengths, are more commonly observed in the far-infrared, in particular toward strong dust continuum sources. The lowest energy transitions are not only observed at LSR-velocities related to the source, but often also at velocities associated with diffuse molecular clouds along the line of sight toward the background source. Unbiased spectral line surveys of the massive and very luminous Galactic Center sources Sagittarius B2(M) and (N) were carried out across the entire frequency range of the high-resolution Heterodyne Instrument for Far-Infrared Astronomy (HIFI). An absorption feature was detected toward both sources at about 617.531 GHz, corresponding to 20.599 cm-1, 485.47 μm, or 2.5539 meV. This feature is unique in its appearance at all velocity components associated with diffuse foreground molecular clouds, together with its conspicuous absence at velocities related to the sources themselves. The carriers of at least a substantial part of the DIBs are thought to reside in the diffuse interstellar medium. Therefore, we consider this absorption feature to be a far-infrared DIB analog. Subsequent dedicated observations confirmed that the line is present only in the foreground clouds on the line of sight toward other massive star-forming regions in the Galactic disk. There is indication that the feature has substructure, possibly of fine or hyperfine nature. Attempts to assign the feature to atomic or molecular species have been unsuccessful so far.},
	keywords = {Ism: clouds; Line: identification; submillimeter: ISM; ISM: lines and bands},
	year = {2014},
	pages = {197-202}
}

@article{MTMT:24136950,
	title = {Asteroseismology, standard candles and the Hubble Constant: what is the role of asteroseismology in the era of precision cosmology?},
	url = {https://m2.mtmt.hu/api/publication/24136950},
	author = {Neilson, Hilding R and Biesiada, Marek and Evans, Nancy Remage and Marconi, Marcella and Ngeow, Chow-Choong and Reese, Daniel R},
	doi = {10.1017/S1743921313014385},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {9},
	unique-id = {24136950},
	issn = {0074-1809},
	year = {2014},
	pages = {233-240}
}

@article{MTMT:24136949,
	title = {Blazhko effect in Cepheids and RR Lyrae stars},
	url = {https://m2.mtmt.hu/api/publication/24136949},
	author = {Szabó, Róbert},
	doi = {10.1017/S1743921313014397},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {9},
	unique-id = {24136949},
	issn = {0074-1809},
	year = {2014},
	pages = {241-248}
}

@article{MTMT:22312492,
	title = {Modulated Light Curves of Multiperiodic Stars},
	url = {https://m2.mtmt.hu/api/publication/22312492},
	author = {Benkő, JM and Szabó, R and Paparó, M},
	doi = {10.1017/S1743921312000804},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {282},
	unique-id = {22312492},
	issn = {0074-1809},
	year = {2012},
	pages = {139}
}

@article{MTMT:26702669,
	title = {Asteroseismic observations of OB stars},
	url = {https://m2.mtmt.hu/api/publication/26702669},
	author = {De Cat, Peter and Uytterhoeven, Katrien and Gutierrez-Soto, Juan and Degroote, Pieter and Simon-Diaz, Sergio},
	doi = {10.1017/S1743921311011070},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {272},
	unique-id = {26702669},
	issn = {0074-1809},
	year = {2011},
	pages = {433-444},
	orcid-numbers = {Gutierrez-Soto, Juan/0000-0001-6736-0551}
}

@article{MTMT:25259287,
	title = {Interior structure models of terrestrial exoplanets and application to CoRoT-7 b},
	url = {https://m2.mtmt.hu/api/publication/25259287},
	author = {Wagner, Frank W and Sohl, Frank and Rauer, Heike and Hussmann, Hauke and Grott, Matthias},
	doi = {10.1017/S1743921310011105},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {15},
	unique-id = {25259287},
	issn = {0074-1809},
	year = {2010},
	pages = {708-709}
}

@article{MTMT:23856449,
	title = {Do Low Luminosity Stars Matter?},
	url = {https://m2.mtmt.hu/api/publication/23856449},
	author = {Ruiz, María Teresa},
	doi = {10.1017/S1743921310008185},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {15},
	unique-id = {23856449},
	issn = {0074-1809},
	year = {2010},
	pages = {47-60}
}

@article{MTMT:1816927,
	title = {Harmonic analysis approach to solar cycle prediction and the Waldmeier effect},
	url = {https://m2.mtmt.hu/api/publication/1816927},
	author = {Petrovay, Kristóf},
	doi = {10.1017/S1743921309992560},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {264},
	unique-id = {1816927},
	issn = {0074-1809},
	abstract = {It is demonstrated that, in addition to the precursor method, harmonic analysis approach to solar cycle prediction is also strongly conditioned by the Waldmeier effect.},
	keywords = {Sun: activity},
	year = {2010},
	pages = {150-154},
	orcid-numbers = {Petrovay, Kristóf/0000-0002-1714-2027}
}

@article{MTMT:20863230,
	title = {Deep Astrometric Standards},
	url = {https://m2.mtmt.hu/api/publication/20863230},
	author = {Platais, I and Fey, A L and Frey, S and Djorgovski, S G and Ducourant, C and Ivezić, Ž and Rest, A and Veillet, C and Wyse, R F R and Zacharias, N},
	doi = {10.1017/S1743921308019455},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {248},
	unique-id = {20863230},
	issn = {0074-1809},
	year = {2008},
	pages = {320-323}
}

@article{MTMT:21204707,
	title = {On the dynamics of Trojan planets in extrasolar planetary systems},
	url = {https://m2.mtmt.hu/api/publication/21204707},
	author = {Dvorak, R and Schwarz, R and Lhotka, Ch},
	doi = {10.1017/S1743921308016979},
	journal-iso = {IAU SYMP},
	journal = {INTERNATIONAL ASTRONOMICAL UNION. PROCEEDINGS OF SYMPOSIA},
	volume = {3},
	unique-id = {21204707},
	issn = {0074-1809},
	year = {2008},
	pages = {461-468}
}