... Strong fossil hypothesis For M >2 M, stars continue to accrete mass and magnetic flux after they have developed a radiative ...
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46. casacore: casa::MRBase Class Reference
... Definition at line 103 of file MRBase.h . virtual casa::MRBase::~MRBase . ( . ) . [virtual] . virtual Bool casa::MRBase::empty . ...
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49. http://www.atnf.csiro.au/research/Astro2010/talks/roy.pdf
... V difference image made from data integrated between 35 to 103 and 103 to 155 seconds respectively from the scan start and ... if their K7V star is replaced by a ~0.1.M star ~0.1 Gyr old (young mid to late M type of star) with Av ~3.5 (distance ~4 kpc ...
50. HIPASS Bright Galaxy Catalog
... 5.7 887.8 17.6 66.1 97.8 EXA 11 09:41:04 -60:30:32 new 0.103 5.5 3073.6 15.5 62.6 110.9 HIP 411 09:44:44 -31:49:02 UGCA180_IC2507 v=1250 ; 09-07-2001, ?m, more needed HIP 459 10:43:06 -36:23:25 group-NGC3354 v=2994 ; 09-07-2001, ?m, more needed ADD 335 11 ...