[et_pb_section bb_built="1"][et_pb_row][et_pb_column type="4_4"][et_pb_text _builder_version="3.15"]
M65 is part of the Leo triplet along with M66 and NGC3628. The galaxy is low in dust and gas, and there is little star formation in it, although there has been some relatively recently in the arms. The ratio of old stars to new stars is correspondingly quite high. In most wavelengths it is quite uninteresting, though there is a radio source visible in the NVSS, offset from the core by about two arc-minutes. The identity of the source is uncertain, as it has not been identified visually, or formally studied in any published papers.
[/et_pb_text][/et_pb_column][/et_pb_row][et_pb_row][et_pb_column type="4_4"][et_pb_text admin_label="Martin Crow" _builder_version="3.15"]
Images by Martin Crow
[/et_pb_text][/et_pb_column][/et_pb_row][et_pb_row][et_pb_column type="1_4"][et_pb_text admin_label="MC Image" _builder_version="3.15"]
[/et_pb_text][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][/et_pb_row][et_pb_row][et_pb_column type="4_4"][et_pb_text admin_label="Julian Tworek" _builder_version="3.15"]
Images by Julian Tworek
[/et_pb_text][/et_pb_column][/et_pb_row][et_pb_row][et_pb_column type="1_4"][et_pb_text admin_label="JT Image" _builder_version="3.15"]
[/et_pb_text][/et_pb_column][et_pb_column type="1_4"][et_pb_text admin_label="JT Image" _builder_version="3.15"]
[/et_pb_text][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][/et_pb_row][et_pb_row][et_pb_column type="4_4"][et_pb_text admin_label="Andrew Wilson" _builder_version="3.15"]
Images by Andrew Wilson
[/et_pb_text][/et_pb_column][/et_pb_row][et_pb_row][et_pb_column type="1_4"][et_pb_text admin_label="AW Image" _builder_version="3.15"]
[/et_pb_text][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][et_pb_column type="1_4"][/et_pb_column][/et_pb_row][/et_pb_section]
