id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2358	Panagia, Nino; De Marchi, Guido	Star Formation as Seen by Low Mass Stars	2014	5	.pdf	application/pdf	2273	75	58	Our motivations are: i) Stars in this range account for most of the star formation in a galaxy, e.g. more than 65% for a Salpeter initial mass function (IMF); ii) Low mass stars can form in small parent clouds as well as in big ones; iii) As a consequence, low mass stars are forming near massive stars as well as in isolated groups. 114 Star Formation as Seen by Low Mass Stars Figure 3: The left panel shows the mass accretion rate as a function of stellar age for PMS stars in NGC 346 (diamonds) compared with that of Galactic T Tauri stars (see legend) from the work of Sicilia–Aguilar et al. (2006; the large cross indicates the uncertainties as quoted in that paper).	cache/app01-2358.pdf	txt/app01-2358.txt