TY - JOUR
T1 - A three-decade outburst of the lmc luminous blue variable R127 draws to a close
AU - Walborn, Nolan R.
AU - Stahl, Otmar
AU - Gamen, Roberto C.
AU - Szeifert, Thomas
AU - Morrell, Nidia I.
AU - Smith, Nathan
AU - Howarth, Ian D.
AU - Humphreys, Roberta M.
AU - Bond, Howard E.
AU - Lennon, Daniel J.
PY - 2008
Y1 - 2008
N2 - The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the inter-mediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are characterized by multiple spikes and dips, which may provide constraints on the unknown outburst mechanism. Intensive photometric and spec-troscopic monitoring of R127 should now resume, to follow the decline presumably back to the quiescent Ofpe/WN9 state, in order to fully document the remainder of this unique observational opportunity.
AB - The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the inter-mediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are characterized by multiple spikes and dips, which may provide constraints on the unknown outburst mechanism. Intensive photometric and spec-troscopic monitoring of R127 should now resume, to follow the decline presumably back to the quiescent Ofpe/WN9 state, in order to fully document the remainder of this unique observational opportunity.
UR - http://www.scopus.com/inward/record.url?scp=62649095567&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=62649095567&partnerID=8YFLogxK
U2 - 10.1086/592110
DO - 10.1086/592110
M3 - Article
AN - SCOPUS:62649095567
SN - 0004-637X
VL - 684
SP - L33-L36
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1 PART 2
ER -