Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Thomasson, Magnus"'
Autor:
Zinchenko, Igor I., Pazukhin, Andrey G., Trofimova, Elena A., Zemlyanukha, Peter M., Henkel, Christian, Thomasson, Magnus
We present the results of our studies of deuterated molecules (DCN, DNC, DCO$^+$, N$_2$D$^+$ and NH$_2$D) in regions of high-mass star formation, which include a survey of such regions with the 20-m Onsala radio telescope and mapping of several objec
Externí odkaz:
http://arxiv.org/abs/2209.07832
Autor:
Elmegreen, Debra Meloy, Elmegreen, Bruce G., Kaufman, Michele, Sheth, Kartik, Struck, Curtis, Thomasson, Magnus, Brinks, Elias
IC 2163 and NGC 2207 are interacting galaxies that have been well studied at optical and radio wavelengths and simulated in numerical models to reproduce the observed kinematics and morphological features. Spitzer IRAC and MIPS observations reported
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605524
Autor:
Struck, Curtis, Kaufman, Michele, Brinks, Elias, Thomasson, Magnus, Elmegreen, Bruce G., Elmegreen, Debra Meloy
Publikováno v:
Mon.Not.Roy.Astron.Soc.364:69-90,2005
We present numerical hydrodynamical models of the collision between the galaxies IC 2163 and NGC 2207. These models extend the results of earlier work where the galaxy discs were modeled one at a time. We confirm the general result that the collision
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508660
Autor:
Kaufman, Michele, Sheth, Kartik, Struck, Curtis, Elmegreen, Bruce G., Thomasson, Magnus, Elmegreen, Debra Meloy, Brinks, Elias
BIMA CO 1-0 observations are presented of the spiral galaxies NGC 5394 and NGC 5395 that have undergone a recent, grazing encounter. In NGC 5394, 80% of the CO emission detected by BIMA is concentrated in the central 800 pc (FWHM) starburst region.In
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111240
Autor:
Kirsanova Maria S., Salii Svetlana V., Sobolev Andrej M., Olofsson Anders Olof Henrik, Ladeyschikov Dmitry A., Thomasson Magnus
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 99-105 (2017)
We studied the distribution of dense gas in a filamentary molecular cloud containing several dense clumps. The center of the filament is given by the dense clump WB673. The clumps are high-mass and intermediate-mass starforming regions. We observed C
Externí odkaz:
https://doaj.org/article/9552c9c4a17a406b97c9045fc49005f7
Autor:
Meloy, Debra, Elmegreen, Bruce G., Kaufman, Michele, Sheth, Kartik, Struck, Curtis, Thomasson, Magnus, Brinks, Elias
Publikováno v:
The Astrophysical Journal; May 2006, Vol. 642 Issue: 1 p158-170, 13p
Autor:
Elmegreen, Debra Meloy, Elmegreen, Bruce G., Kaufman, Michele, Sheth, Kartik, Struck, Curtis, Thomasson, Magnus, Brinks, Elias
Publikováno v:
Astrophysical Journal; 5/1/2006, Vol. 642 Issue 1, p1-1, 1p
Autor:
Kaufman, Michele, Sheth, Kartik, Struck, Curtis, Elmegreen, Bruce G., Thomasson, Magnus, Elmegreen, Debra Meloy, Brinks, Elias
Publikováno v:
Astronomical Journal; Feb2002, Vol. 123 Issue 2, p1-1, 1p
Autor:
Elmegreen, Debra Meloy, Kaufman, Michele, Elmegreen, Bruce G., Brinks, Elias, Struck, Curtis, Klarić, Mario, Thomasson, Magnus
Publikováno v:
Astronomical Journal; Jan2001, Vol. 121 Issue 1, p1-1, 1p
Autor:
Elmegreen, Bruce G., Kaufman, Michele, Struck, Curtis, Elmegreen, Debra Meloy, Brinks, Elias, Thomasson, Magnus, Klarić, Mario, Levay, Zolt, English, Jayanne, Frattare, L. M., Bond, Howard E., Christian, C. A., Hamilton, F., Noll, K.
Publikováno v:
Astronomical Journal; Dec2000, Vol. 120 Issue 6, p1-1, 1p