Results 31 to 40 of about 68,608 (160)

THE ABUNDANCES OF THE ELEMENTS OF THE MAGELLANIC CLOUDS

Odessa Astronomical Publications, 2010
The results of the spectroscopic researches of classical Chepheids of the Magellanic Clouds (MC) are presented in this paper. 21 spec tra for the Large Magellanic Cloud (LMC) and 10 for the Small Magellanic Cloud (SMC) were investigated.
F. A. Chekhonadskikh
doaj   +1 more source

Discovery of 14 radio pulsars in a survey of the Magellanic Clouds [PDF]

, 2006
A systematic survey of the Large and Small Magellanic Clouds for radio pulsars using the Parkes radio telescope and the 20-cm multibeam receiver has resulted in the discovery of 14 pulsars and the redetection of five of the eight previously known spin ...
Crawford, Fronefield, Fan, G., Kaspi, V. M., Lyne, A. G., Manchester, R. N.   +4 more
core   +3 more sources

The Parkes HI Survey of the Magellanic System [PDF]

Astron.Astrophys.432:45-67,2005, 2004
We present the first fully and uniformly sampled, spatially complete HI survey of the entire Magellanic System with high velocity resolution, performed with the Parkes Telescope. The final data-cubes have an rms noise of sigma ~ 0.05 K and an effective angular resolution of 16 arcmin. The Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC)
arxiv   +1 more source

Sub-millimeter to centimeter excess emission from the Magellanic Clouds. I. Global spectral energy distribution [PDF]

, 2010
In order to reconstruct the global SEDs of the Magellanic Clouds over eight decades in spectral range, we combined literature flux densities representing the entire LMC and SMC respectively, and complemented these with maps extracted from the WMAP and ...
Agladze, Aguirre, Ali-Haïmoud, Alvarez, Alvarez, Alvarez, Beirão, Bell, Bendo, Bennett, Bennett, Bernard, Boggess, Bolatto, C. Bot, Caplan, Chen, D. Raban, Dicker, Dobler, Draine, Draine, Dumke, Dupac, Engelbracht, F. P. Israel, Fixsen, Fixsen, Galliano, Galliano, Haynes, Hinshaw, Hughes, Hunt, Israel, J. B. R. Oonk, J. P. Bernard, Kennicutt, Klein, Leroy, Lisenfeld, Loiseau, Mathis, Mennella, Mountfort, Murphy, Mény, N. Ysard, Ossenkopf, Page, Paradis, Reach, Rice, Sakon, Schlegel, Silverberg, Smith, Stanimirovic, Vacca, W. F. Wall, W. T. Reach, Wall, Wilke, Wright, Ye, Ysard, Ysard, Zhu   +67 more
core   +5 more sources

MACHO 311.37557.169: A VY Scl star

Astronomische Nachrichten, Volume 341, Issue 3, Page 283-290, March 2020., 2020
Abstract Optical surveys, such as the MACHO project, often uncover variable stars whose classification requires follow‐up observations by other instruments. We performed X‐ray spectroscopy and photometry of the unusual variable star MACHO 311.37557.169 with XMM‐Newton in April 2018, supplemented by archival X‐ray and optical spectrographic data.
Hauke Wörpel, Axel D. Schwope, Iris Traulsen, Michael J. I. Brown   +3 more
wiley   +1 more source

Stellar dust production and composition in the Magellanic Clouds [PDF]

, 2012
The dust reservoir in the interstellar medium of a galaxy is constantly being replenished by dust formed in the stellar winds of evolved stars. Due to their vicinity, nearby irregular dwarf galaxies the Magellanic Clouds provide an opportunity to obtain ...
Kemper, F.
core   +2 more sources

Auch Sterne altern

Physik in unserer Zeit, Volume 51, Issue 2, Page 88-95, March 2020., 2020
Das Alter des Universums und der Sterne zu ermitteln, gehört seit jeher zu den zentralen Aufgaben der Astrophysik. Mittlerweile gibt es hierfür eine Vielzahl von Methoden. Einige liefern erstaunlich genaue Werte, andere sind unsicherer. Was also wissen wir heute und mit welcher Genauigkeit über das Alter von Sternen?
Achim Weiss
wiley   +1 more source

Supernova remnants in nearby galaxies

Astronomische Nachrichten, Volume 341, Issue 2, Page 156-162, February 2020., 2020
Abstract Supernova remnants (SNRs) are the aftermath of stellar explosions, which inject large amounts of energy into the interstellar medium (ISM), carving out new structures and transferring kinetic energy to the ISM. They also act as recycling centers, which return elements processed in stars to the ISM, and cosmic particle accelerators.
Manami Sasaki
wiley   +1 more source

Pulsating stars in the VMC survey

EPJ Web of Conferences, 2017
The VISTA survey of the Magellanic Clouds system (VMC) began observations in 2009 and since then, it has collected multi-epoch data at Ks and in addition multi-band data in Y and J for a wide range of stellar populations across the Magellanic system ...
Cioni Maria-Rosa L., Ripepi Vincenzo, Clementini Gisella, Groenewegen Martin A.T., Moretti Maria I., Muraveva Tatiana, Subramanian Smitha   +6 more
doaj   +1 more source

Astrophysical Distance Scale. VII. A Self-consistent, Multiwavelength Calibration of the Slopes and Relative Zero Points for the Run of Luminosity with the Color of Stars Defining the Tip of the Red Giant Branch

The Astronomical Journal, 2023
Given the recent successful launch of the James Webb Space Telescope, determining robust calibrations of the slopes and absolute magnitudes of the near- to mid-infrared tip of the red-giant branch (TRGB) will be essential to measuring precise ...
Barry F. Madore, Wendy L. Freedman, Kayla Owens   +2 more
doaj   +1 more source