Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Tatiana Vasyunina"'
Publikováno v:
Proceedings of the International Astronomical Union. 6:455-458
The determination of prestellar core structure is often based on observations of (sub)millimeter dust continuum. However, recently the Spitzer Space Telescope provided us with IR images of many objects not only in emission but also in absorption. We
Publikováno v:
Proceedings of the 69th International Symposium on Molecular Spectroscopy.
Autor:
Edwin A. Bergin, Shanshan Yu, Thomas G. Phillips, Trevor D. McNeill, Peter Schilke, Cécile Favre, Justin L. Neill, Claudia Comito, Martin Emprechtinger, Amanda L. Steber, Dariusz C. Lis, Raquel Monje, Andrew M. Burkhardt, Brent J. Harris, Brett A. McGuire, Dana E. Anderson, Sheng-Li Qin, Steven D. Lord, Jo Hsin Chen, Tatiana Vasyunina, Nathan R. Crockett
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2014, 789 (1), pp.8. ⟨10.1088/0004-637X/789/1/8⟩
The Astrophysical Journal, American Astronomical Society, 2014, 789 (1), pp.8. ⟨10.1088/0004-637X/789/1/8⟩
A sensitive broadband molecular line survey of the Sagittarius B2(N) star-forming region has been obtained with the HIFI instrument on the Herschel Space Observatory, offering the first high-spectral resolution look at this well-studied source in a w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::266b56d491fc32134e0d670a0d7c95a7
http://arxiv.org/abs/1405.0706
http://arxiv.org/abs/1405.0706
Autor:
Thomas Henning, Henrik Beuther, Thomas Gerner, Tatiana Vasyunina, Hendrik Linz, Dmitry Semenov
Publikováno v:
The Labyrinth of Star Formation ISBN: 9783319030401
Understanding the chemical evolution of young (high-mass) star-forming regions is a central topic in star formation research. The chemistry plays two main roles here: to study the evolution from simple to complex molecules, and to investigate the und
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1de7da19a3fdabdf74503fd26c78ba5b
https://doi.org/10.1007/978-3-319-03041-8_81
https://doi.org/10.1007/978-3-319-03041-8_81
Autor:
Kelsey E. Johnson, Frédéric Galliano, Tatiana Vasyunina, Suzanne C. Madden, Margaret Meixner, C.-H. Rosie Chen, Erik Muller, Joana M. Oliveira, Amanda A. Kepley, Remy Indebetouw, Crystal L. Brogan, Annie Hughes, Vianney Lebouteiller, Todd R. Hunter, D. Cormier, Toshikazu Onishi, Akiko Kawamura, Adam K. Leroy
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2013, 774 (1), pp.73. ⟨10.1088/0004-637X/774/1/73⟩
The Astrophysical Journal, American Astronomical Society, 2013, 774 (1), pp.73. ⟨10.1088/0004-637X/774/1/73⟩
The Astrophysical Journal, 2013, 774 (1), pp.73. ⟨10.1088/0004-637X/774/1/73⟩
The Astrophysical Journal, American Astronomical Society, 2013, 774 (1), pp.73. ⟨10.1088/0004-637X/774/1/73⟩
We present ALMA observations of 30 Doradus -- the highest resolution view of molecular gas in an extragalactic star formation region to date (~0.4pc x 0.6pc). The 30Dor-10 cloud north of R136 was mapped in 12CO 2-1, 13CO 2-1, C18O 2-1, 1.3mm continuu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb67ede65516039c777ed0a8236c117a
Autor:
Sarah Ragan, Tatiana Vasyunina, J. Tackenberg, Henrik Beuther, Oliver Krause, Hendrik Linz, Jan Pitann, Amelia M. Stutz, Ralf Launhardt, Thomas Henning, Anika Schmiedeke, Frederic Schuller
We present continuum observations of the infrared dark cloud (IRDC) G48.66-0.22 (G48) obtained with Herschel, Spitzer, and APEX, in addition to several molecular line observations. The Herschel maps are used to derive temperature and column density m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3de223a292fce0387cd466e6f56499bb
Autor:
Anika Schmiedeke, Markus Nielbock, Henrik Beuther, Oliver Krause, Ralf Launhardt, Zoltan Balog, Jan Pitann, Martin Hennemann, N. Lippok, Hendrik Linz, J. Tackenberg, Tatiana Vasyunina, Sarah Ragan, Juergen Steinacker, Thomas Henning, Amelia M. Stutz, Frederic Schuller
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2012, 547, pp.A49. ⟨10.1051/0004-6361/201219232⟩
Astronomy and Astrophysics-A&A, 2012, 547, pp.A49. ⟨10.1051/0004-6361/201219232⟩
(Abridged) We present an overview of the sample of high-mass star and cluster forming regions observed as part of the Earliest Phases of Star Formation (EPoS) Herschel Guaranteed Time Key Program. A sample of 45 infrared-dark clouds (IRDCs) were mapp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b0c6187a1eb8164bc028a44b204e67d
https://orca.cardiff.ac.uk/id/eprint/106500/1/aa19232-12.pdf
https://orca.cardiff.ac.uk/id/eprint/106500/1/aa19232-12.pdf
Autor:
Sarah Ragan, Oliver Krause, Hendrik Linz, Markus Nielbock, Tatiana Vasyunina, Ralf Launhardt, Henrik Beuther, Thomas Henning
Infrared-dark clouds (IRDCs) are the precursors to massive stars and stellar clusters. G011.11-0.12 is a well-studied filamentary IRDC, though, to date, the absence of far-infrared data with sufficient spatial resolution has limited the understanding
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5b26635e499497bb6d4cb065c4e2fbd
Autor:
Jonathan B. Foster, Andrés E. Guzmán, Jill Rathborne, Tatiana Vasyunina, Christopher Claysmith, J. Scott Whitaker, Patricio Sanhueza, James M. Jackson, Sadia Hoq, Anton Vasyunin
Publikováno v:
Astrophysical Journal
The chemical changes of high-mass star-forming regions provide a potential method for classifying their evolutionary stages and, ultimately, ages. In this study, we search for correlations between molecular abundances and the evolutionary stages of d