Tag: primary background

Documents tagged

hot massive stars

Documents Discovery of xray_emission_from_young_suns_in_the_small_magellaniccloud

1. Draft version January 17, 2013Preprint typeset using L TEX style emulateapj v. 5/2/11 ADISCOVERY OF X-RAY EMISSION FROM YOUNG SUNS IN THE SMALL MAGELLANIC CLOUD L. M.…

Documents Active star formation_in_n11

1. Active star formation in N11B Nebula in the Large MagellanicCloud: a sequential star formation scenario conﬁrmed 1 2Rodolfo H. Barb´3 aObservatorio Astron´mico La…

Documents Cosmology 2002/2003 - March1 The Luminosity Function See Math in Tecra 8100 Thanks for Dr. Paolo...

The Luminosity Function See Math in Tecra 8100 Thanks for Dr. Paolo Saracco for the example of the L.F. Estimate with Vmax to Tagliaferri for catching some typos – Ref.…

Documents Stellar Evolution Stars evolve (change over time) because of GRAVITY! A star passes through phases,....

Stellar Evolution Stars evolve (change over time) because of GRAVITY! A star passes through phases, grouped as Pre-Main Seq (birth) Main Seq (MS) (life) Post-MS (demise)…

Documents By Guido Chincarini H o =50 km/s/Mpc L * =3.2 10 10 L = -1.25 Mv =-26.78 Mbol =-26.85

The Luminosity Function See Math in Tecra 8100 Thanks for Dr. Paolo Saracco for the example of the L.F. Estimate with Vmax to Tagliaferri for catching some typos – Ref.…