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Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars
R. Unnikrishnan, M. Andriantsaralaza, E. De Beck, L.-Å. Nyman, H. Olofsson, W. H. T. Vlemmings, M. Maercker, M. Van de Sande, T. Danilovich, T. J. Millar, S. B. Charnley and M. G. Rawlings Astronomy & Astrophysics 699 A48 (2025) https://doi.org/10.1051/0004-6361/202554996
A brief introduction of chemistry in the disks of protoplanetary nebulae
B-G. Andersson, Janik Karoly, Pierre Bastien, Archana Soam, Simon Coudé, Mehrnoosh Tahani, Michael S. Gordon and Sydney Fox-Middleton The Astrophysical Journal 963(1) 76 (2024) https://doi.org/10.3847/1538-4357/ad1835
Modelling predicts a molecule-rich disc around the AGB star L2 Puppis
M Van de Sande, C Walsh, T Danilovich, F De Ceuster and T Ceulemans Monthly Notices of the Royal Astronomical Society 532(1) 734 (2024) https://doi.org/10.1093/mnras/stae1553
Molecular line polarisation from the circumstellar envelopes of asymptotic giant branch stars
Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars
R. Unnikrishnan, E. De Beck, L.-Å. Nyman, H. Olofsson, W. H. T. Vlemmings, D. Tafoya, M. Maercker, S. B. Charnley, M. A. Cordiner, I. de Gregorio, E. Humphreys, T. J. Millar and M. G. Rawlings Astronomy & Astrophysics 684 A4 (2024) https://doi.org/10.1051/0004-6361/202346264
Disentangling physics and chemistry in AGB outflows: revealing degeneracies when adding complexity
Investigating Anomalous Photochemistry in the Inner Wind of IRC+10216 through Interferometric Observations of HC3N
Mark A. Siebert, Marie Van de Sande, Thomas J. Millar and Anthony J. Remijan The Astrophysical Journal 941(1) 90 (2022) https://doi.org/10.3847/1538-4357/ac9e52
Multifrequency high spectral resolution observations of HCN toward the circumstellar envelope of Y Canum Venaticorum
Multiepoch Optical Images of IRC+10216 Tell about the Central Star and the Adjacent Environment
Hyosun Kim, Ho-Gyu Lee, Youichi Ohyama, Ji Hoon Kim, Peter Scicluna, You-Hua Chu, Nicolas Mauron and Toshiya Ueta The Astrophysical Journal 914(1) 35 (2021) https://doi.org/10.3847/1538-4357/abf6cc
Fine-grained distributed averaging for large-scale radio interferometric measurement sets
The Maser-emitting Structure and Time Variability of the SiS Lines J = 14–13 and 15–14 in IRC+10216*
J. P. Fonfría, M. Fernández-López, J. R. Pardo, M. Agúndez, C. Sánchez Contreras, L. Velilla Prieto, J. Cernicharo, M. Santander-García, G. Quintana-Lacaci, A. Castro-Carrizo and S. Curiel The Astrophysical Journal 860(2) 162 (2018) https://doi.org/10.3847/1538-4357/aac5e3
The VLTI/MIDI view on the inner mass loss of evolved stars from theHerschelMESS sample
The weather report from IRC+10216: evolving irregular clouds envelop carbon star
P. N. Stewart, P. G. Tuthill, J. D. Monnier, et al. Monthly Notices of the Royal Astronomical Society 455(3) 3102 (2016) https://doi.org/10.1093/mnras/stv2454
HINTS OF A ROTATING SPIRAL STRUCTURE IN THE INNERMOST REGIONS AROUND IRC +10216
G. Quintana-Lacaci, J. Cernicharo, M. Agúndez, L. Velilla Prieto, A. Castro-Carrizo, N. Marcelino, C. Cabezas, I. Peña, J. L. Alonso, J. Zúñiga, A. Requena, A. Bastida, Y. Kalugina, F. Lique and M. Guélin The Astrophysical Journal 818(2) 192 (2016) https://doi.org/10.3847/0004-637X/818/2/192
Discovery of a shell of neutral atomic hydrogen surrounding the carbon star IRC+10216
L. D. Matthews, E. Gérard and T. Le Bertre Monthly Notices of the Royal Astronomical Society 449(1) 220 (2015) https://doi.org/10.1093/mnras/stv263
ALMA data suggest the presence of spiral structure in the inner wind of CW Leonis
The complex dust formation zone of the AGB star IRC+10216 probed with CARMA 0.25 arcsec angular resolution molecular observations
J. P. Fonfría, M. Fernández-López, M. Agúndez, et al. Monthly Notices of the Royal Astronomical Society 445(3) 3289 (2014) https://doi.org/10.1093/mnras/stu1968
Deep optical imaging of asymptotic giant branch circumstellar envelopes
PHOTOCHEMISTRY IN THE INNER LAYERS OF CLUMPY CIRCUMSTELLAR ENVELOPES: FORMATION OF WATER IN C-RICH OBJECTS AND OF C-BEARING MOLECULES IN O-RICH OBJECTS