Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Micelotta, E."'
Autor:
Montillaud, Julien, Juvela, Mika, Vastel, Charlotte, He, J. H., Liu, Tie, Ristorcelli, Isabelle, Eden, David J., Kang, Sung-ju, Kim, Kee-Tae, Koch, Patrick M., Lee, Chang Won, Rawlings, Mark G., Saajasto, Mika, Sanhueza, Patricio, Soam, Archana, Zahorecz, Sarolta, Alina, Dana, Bögner, Rebeka, Cornu, David, Doi, Yasuo, Malinen, Johanna, Marshall, Douglas, Micelotta, E. R., Pelkonen, V. M., Tóth, L. V., Traficante, A., Wang, Ke
Publikováno v:
A&A 631, A3 (2019)
We started a multi-scale analysis of G202.3+2.5, an intertwined filamentary region of Monoceros OB1. In Paper I, we examined the distributions of dense cores and protostars and found enhanced star formation (SF) activity in the junction region of the
Externí odkaz:
http://arxiv.org/abs/1909.06145
Autor:
Montillaud, Julien, Juvela, Mika, Vastel, Charlotte, He, J. H., Liu, Tie, Ristorcelli, Isabelle, Eden, David J., Kang, Sung-ju, Kim, Kee-Tae, Koch, Patrick M., Lee, Chang Won, Rawlings, Mark G., Saajasto, Mika, Sanhueza, Patricio, Soam, Archana, Zahorecz, Sarolta, Alina, Dana, Bögner, Rebeka, Cornu, David, Doi, Yasuo, Malinen, Johanna, Marshall, Douglas, Micelotta, E. R., Pelkonen, V. M., Tóth, L. V., Traficante, A., Wang, Ke
Publikováno v:
A&A 631, L1 (2019)
Current theories and models attempt to explain star formation globally, from core scales to giant molecular cloud scales. A multi-scale observational characterisation of an entire molecular complex is necessary to constrain them. We investigate star
Externí odkaz:
http://arxiv.org/abs/1909.03781
Autor:
Alina, D., Ristorcelli, I., Montier, L., Abdikamalov, E., Juvela, M., Ferrière, K., Bernard, J. -Ph., Micelotta, E. R.
We present a statistical study of the relative orientation in the plane of the sky between interstellar magnetic fields and filaments hosting cold clumps. For the first time, we consider both the density of the environment and the density contrast be
Externí odkaz:
http://arxiv.org/abs/1712.09325
Autor:
Bernard-Salas, J., Cami, J., Jones, A. P., Peeters, E., Micelotta, E. R., Otsuka, M., Sloan, G. C., Kemper, F., Groenewegen, M.
Publikováno v:
Proceedings of Science (LDCU 2013)032
Fullerenes are a particularly stable class of carbon molecules in the shape of a hollow sphere or ellipsoid that might be formed in the outflows of carbon stars. Once injected into the interstellar medium (ISM), these stable species survive and are t
Externí odkaz:
http://arxiv.org/abs/1407.0962
Autor:
Bernard-Salas, J., Cami, J., Peeters, E., Jones, A. P., Micelotta, E. R., Groenewegen, M. A. T.
We compare and analyze the Spitzer mid-infrared spectrum of three fullerene-rich planetary nebulae in the Milky Way and the Magellanic Clouds; Tc1, SMP SMC16, and SMP LMC56. The three planetary nebulae share many spectroscopic similarities. The stron
Externí odkaz:
http://arxiv.org/abs/1207.5794
Publikováno v:
Astronomy and Astrophysics, 2011, Volume 526, A52
Context: Cosmic rays are present in almost all phases of the ISM. PAHs and cosmic rays represent an abundant and ubiquitous component of the interstellar medium. However, the interaction between them has never before been fully investigated. Aims: To
Externí odkaz:
http://arxiv.org/abs/1012.1599
Publikováno v:
Astron.Astrophys.510:A37,2010
Context: PAHs are thought to be a ubiquitous and important dust component of the interstellar medium. However, the effects of their immersion in a hot (post-shock) gas have never before been fully investigated. Aims: We study the effects of energetic
Externí odkaz:
http://arxiv.org/abs/0912.1595
Publikováno v:
Astron.Astrophys.510:A36,2010
Context: PAHs appear to be an ubiquitous interstellar dust component but the effects of shocks waves upon them have never been fully investigated. Aims: To study the effects of energetic (~0.01-1 keV) ion (H, He and C) and electron collisions on PAHs
Externí odkaz:
http://arxiv.org/abs/0910.2461
Publikováno v:
Astron.Astrophys.500:807-815,2009
(Aims): We study the LMC interstellar medium in the field of the nebula N157B, which contains a supernova remnant, an OB association, ionized gas, and high-density dusty filaments in close proximity. We investigate the relative importance of shock ex
Externí odkaz:
http://arxiv.org/abs/0907.0004
Autor:
Micelotta, E. R.1 (AUTHOR) elisabetta.micelotta@helsinki.fi, Matsuura, M.2 (AUTHOR) MatsuuraM@cardiff.ac.uk, Sarangi, A.3,4 (AUTHOR) arkaprabha.sarangi@nasa.gov
Publikováno v:
Space Science Reviews. Mar2018, Vol. 214 Issue 2, p1-8. 8p.
