... The project has been inspired by the recent Arecibo detection of the prebiotic molecule, methanimine (CH2NH) in the protypical ULIRG/megamaser galaxy, Arp220 (Salter et al. ...
... The project has been inspired by the recent Arecibo detection of the prebiotic molecule, methanimine (CH2NH) in the protypical ULIRG/megamaser galaxy, Arp220 (Salter et al. ...
... The project has been inspired by the recent Arecibo detection of the prebiotic molecule, methanimine (CH2NH) in the protypical ULIRG/megamaser galaxy, Arp220 (Salter et al. ...
... The project has been inspired by the recent Arecibo detection of the prebiotic molecule, methanimine (CH2NH) in the protypical ULIRG/megamaser galaxy, Arp220 (Salter et al. ...
... Plots - one for line (left) and one for continuum (right) sensitivity versus the exp ected SED of a high z star forming galaxy with a luminosity 1/10 that of arp220 - this would b e typical of Lyman break galaxies or Lyman alpha galaxies. ...
... P.E. Robinson, A. Saintonge, S.T. Strasser, and C.J. Salter, High Sensitivity Observations of the Satellite OH Lines of Arp220, American Astronomical Society Meeting 203, #115.08, Dec 2003 Giovanelli, R., M.P. Haynes, K. Spekkens, C.M. Springob, K.L ...
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Ссылки http://www.naic.edu/~astro/NSFSR/NAIC_Publication_Statistics.pdf -- 713.3 Кб -- 20.09.2005 Похожие документы
... the highest resolution radar imThe supernova rate in the prototypical ages ever made of the moon, planetary ultraluminous infrared galaxy Arp220 astronomers found no evidence for ice has been measured by means of VLBI in the craters at the lunar south ...
... That time a computer using the "other" part of the subnet sent arp packets saying that they also belonged to the "cor backplane ... Tsys is about 151 K. There is a 220 second ripple in the cal . 27aug05: lbw . ...
... toward Galactic center, Y in direction of Galactic rotation, Z toward North Galactic Pole ID Name RA (2000) DEC L B R_Sun R_gc X Y Z NGC 104 47 Tuc 00 24 05.2 -72 04 51 305.90 -44.89 4.5 7.4 1.9 -2.6 -3.2 NGC 288 00 52 47.5 -26 35 24 152.28 -89...