Results 121 to 130 of about 167,903 (283)

Stellar Population near NGC 2021: Procession of Star Formation in the South Rim of Supergiant Shell LMC 4

The Astronomical Journal
Supergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy’s halo. The SGSs in the Large Magellanic Cloud (LMC) are so close that their stars can be resolved with ground-based telescopes to ...
Po-Sheng Ou, Rui-Ching Chao, You-Hua Chu, Chin-Yi Hsu, Chuan-Jui Li   +4 more
doaj   +1 more source

SPECTRAL LINE SURVEY TOWARD MOLECULAR CLOUDS IN THE LARGE MAGELLANIC CLOUD [PDF]

The Astrophysical Journal, 2016
ABSTRACT Spectral line survey observations of seven molecular clouds in the Large Magellanic Cloud (LMC) have been conducted in the 3 mm band with the Mopra 22 m telescope to reveal chemical compositions in low metallicity conditions. Spectral lines of fundamental species such as CS, SO, CCH, HCN, HCO+, and HNC are detected in addition ...
Yuri Nishimura, Takashi Shimonishi, Yoshimasa Watanabe, Nami Sakai, Yuri Aikawa, Akiko Kawamura, Satoshi Yamamoto   +6 more
openaire   +2 more sources

Properties of the Magellanic Corona

The Astrophysical Journal
We characterize the Magellanic Corona, the warm gaseous halo around the Large Magellanic Cloud (LMC). The Corona is a key ingredient in the formation of the Magellanic Stream and has recently been observed in high-ion absorption around the LMC.
Scott Lucchini, Elena D’Onghia, Andrew J. Fox   +2 more
doaj   +1 more source

The Large Magellanic Cloud R Crb Star — HV12842 [PDF]

International Astronomical Union Colloquium, 1985
The star HV12842 is one of the 5 R CrB stars listed in the catalogue of variable stars in the LMC (Payne-Goposchkin 1971) and is located 4 deg. to the north of 30 Doradus. At this location it falls in the north-eastern part of one of two standard LMC fields used by the UK 1.2 m Schmidt Telescope.
D.H. Morgan, K. Nandy, N. Kameswara Rao
openaire   +1 more source

Large Magellanic Cloud Cepheids in the ASAS data

Acta Astronomica, 2011
A catalog of Cepheids in the Large Magellanic Cloud (LMC) from the ASAS project is presented. It contains data on 65 fundamental mode pulsators with periods longer than about 8 days. The period-luminosity (PL) relation in the V-band does not significantly differ from the relation determined by Soszynski et al.
Karczmarek, P, Dziembowski, W. A, Lenz, P, Pietrukowicz, P, & Pojmański, G.   +4 more
openaire   +2 more sources

Photometric Confirmation of MACHO Large Magellanic Cloud Microlensing Events

, 2005
We present previously unpublished photometry of three Large Magellanic Cloud (LMC) microlensing events and show that the new photometry confirms the microlensing interpretation of these events.
Andrew C. Becker, Ansari R., Austin Tomaney, Beaulieu J. P., Cook K., David P. Bennett, della Valle M., Lasserre T., Udalski A., Udalski A., Woniak P. R.   +10 more
core   +1 more source

ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons [PDF]

, 2020
Hidetoshi Sano, Paul P. Plucinsky, Aya Bamba, Piyush Sharda, M. D. Filipović, Charles J. Law, R. Z. E. Alsaberi, Yumiko Yamane, Kazuki Tokuda, F. Acero, M. Sasaki, Jacco Vink, Tsuyoshi Inoue, Shu‐ichiro Inutsuka, Jiro Shimoda, Kisetsu Tsuge, K. Fujii, F. Voisin, Nigel Maxted, Gavin Rowell, Toshikazu Onishi, Akiko Kawamura, N. Mizuno, Hiroaki Yamamoto, Kengo Tachihara, Y. Fukui   +25 more
openalex   +1 more source

A timing constraint on the (total) mass of the Large Magellanic Cloud [PDF]

, 2015
The research leading to these results has received ERC funding under the programme (FP/2007-2013)/ERC Grant Agreement no. 308024.
J. Peñarrubia, F. G'omez, G. Besla, D. Erkal, Yin-Zhe Ma   +4 more
semanticscholar   +1 more source

JWST Mid-infrared Spectroscopy Resolves Gas, Dust, and Ice in Young Stellar Objects in the Large Magellanic Cloud

The Astrophysical Journal
In this work, we present spectra of 11 young stellar objects (YSOs) taken with the Mid-Infrared Instrument / Medium Resolution Spectroscopy (MRS) instrument on board the James Webb Space Telescope (JWST).
Omnarayani Nayak, Alec S. Hirschauer, Patrick J. Kavanagh, Margaret Meixner, Laurie Chu, Nolan Habel, Olivia C. Jones, Laura Lenkić, Conor Nally, Megan Reiter, Massimo Robberto, B. A. Sargent   +11 more
doaj   +1 more source

Classical Cepheids, what else?

, 2012
We present new and independent estimates of the distances to the Magellanic Clouds (MCs) using near-infrared (NIR) and optical--NIR period--Wesenheit (PW) relations. The slopes of the PW relations are, within the dispersion, linear over the entire period
Bono, G., Genovali, K., Inno, L., Lemasle, B., Matsunaga, N., Primas, F., Romaniello, M.   +6 more
core   +2 more sources