Las nuevas observaciones tambin indican que las dos galaxias estn separadas por unos 30.000 aos luz de distancia y se desplazan a varios cientos de kilmetros por segundo una con respecto a la otra. A medida que sigan interactuando gravitacionalmente, las galaxias van a ir desacelerndose y acercndose, y van a tener varios encuentros ms antes de fusionarse y formar una galaxia elptica masiva. Los astrnomos calculan que este baile tardar unos cientos de millones de aos..
”That’s one thing I don’t get to do very often, because I’d rather help my children with their homework, put them to bed and then order in sushi or pizza or make dinner for my husband.” Her idea of familial bliss? Sporty weekends on Long Island filled with long beach walks, tennis, swimming and sailing. She was groomed from an early age by her grandmother, Est? and her parents, Ronald and Jo Carole, and it was a given that Aerin would rise through the ranks of one of the world’s largest cosmetics companies. But it’s dedication, not privilege, that gives her an edge.
The Hamner families were people of the mountains, settling in a small town called Schuyler, Va. At the turn of the last century. The eldest of a large family, Earl Henry Hamner Jr. Ours is different, she says. Make it ourselves rather than buy a premade crust from, say, Keebler. Our crust is firmer than the Keebler crust, but crumbles just right.
NASHVILLE Tennessee Gov. Bill Haslam is looking into the security of National Guard armories, storefront recruiting facilities, and other installations. The governor issued a directive on Sunday to Tennessee Adjutant Gen. But there was another surprise in the ALMA observations, which did not just discover the carbon monoxide, but also mapped its location in the disc through ALMA’s unique ability to simultaneously measure both position and velocity: the gas is concentrated in a single compact clump. This concentration lies 13 billion kilometers from the star, which is about three times the distance of Neptune from the Sun. Why the gas is in this small clump so far from the star is a mystery.
 The ALMA correlator is one of two such systems in the ALMA complex. ALMA’s total of 66 antennas comprise a main array of 50 antennas (half provided by ESO, and half by NRAO) and an additional, complementary array of 16 antennas called the Atacama Compact Array (ACA), which is provided by the National Astronomical Observatory of Japan (NAOJ). A second correlator, built by the Fujitsu company and delivered by NAOJ, provides independent correlation of the 16 antennas in the ACA, except for times when select ACA antennas are combined with the 50 more widely dispersed main array antennas..