林茨1014

|- style="vertical-align: top;"
| Distance
| 652.32 Ly (200 pc)

林茨1014（Lynds 1014，或稱為LDN 1014），是一個位於天鵝座的暗星雲。它可能是已知的小型暗星雲中核心密度最高的，代表它可能位於恆星形成的最早階段。林茨1014核心中有一顆非常年輕的低質量恆星，稱為 L1014 IRS。部分天文學家認為該星體可能是棕矮星生命中最早的階段。

參考資料
外部連結

• [http://iopscience.iop.org/0004-637X/640/1/391 Deep Near-Infrared Observations of L1014: Revealing the Nature of the Core and Its Embedded Source]
• [http://jumk.de/astronomie/special-stars/l1014.shtml L1014]
• [http://www.stsci.edu/observing/phase2-public/10603.pro HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 10603 Version: 18 Check-in Time: 06-Mar-2007 21:38:55 STScI Edit Number: 1]
• [http://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/full/2005/33/aa2411-04/aa2411-04.fig.html Lynds 1014 All Figures]
• [http://cfa-www.harvard.edu/sirtf-c2d-cfa/CORES-DB/L1014/L1014.html Core L1014]
• [https://web.archive.org/web/20070715051815/http://www.spitzer.caltech.edu/Media/releases/ssc2004-20/ssc2004-20a.shtml The Starless Core That Isn't] // Spitzer Image, Release Date: 11/09/04
• [http://www.nasa.gov/vision/universe/starsgalaxies/spitzer-110904_prt.htm Spitzer Sees Ice and Warm Glows in Dark and Dusty Places] // NASA 11.09.04